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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/ 2004 /

CMFULL0_2004001_01

Start Time:	2004-001T00:02:19.733	Stop Time:	2004-001T23:59:20.171
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004002_01

Start Time:	2004-002T00:02:20.170	Stop Time:	2004-002T23:59:20.607
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004003_01

Start Time:	2004-003T00:02:20.606	Stop Time:	2004-003T23:59:21.043
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_2004004_01

Start Time:	2004-004T00:02:21.042	Stop Time:	2004-004T23:59:21.480
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004005_01

Start Time:	2004-005T00:02:21.479	Stop Time:	2004-005T23:59:21.916
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004006_01

Start Time:	2004-006T00:02:21.915	Stop Time:	2004-006T23:59:22.352
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004007_01

Start Time:	2004-007T00:02:22.351	Stop Time:	2004-007T23:59:21.789
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_2004008_01

Start Time:	2004-008T00:02:21.788	Stop Time:	2004-008T23:59:22.225
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004009_01

Start Time:	2004-009T00:02:22.224	Stop Time:	2004-009T23:58:21.787
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_2004010_01

Start Time:	2004-010T00:02:21.785	Stop Time:	2004-010T23:58:23.223
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_2004011_01

Start Time:	2004-011T00:02:23.222	Stop Time:	2004-011T23:58:24.660
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004012_01

Start Time:	2004-012T00:02:24.658	Stop Time:	2004-012T23:58:26.096
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004013_01

Start Time:	2004-013T00:02:26.094	Stop Time:	2004-013T23:58:27.532
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004014_01

Start Time:	2004-014T00:02:27.531	Stop Time:	2004-014T23:58:29.969
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_2004015_01

Start Time:	2004-015T00:02:29.967	Stop Time:	2004-015T23:58:31.405
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004016_01

Start Time:	2004-016T00:02:31.403	Stop Time:	2004-016T23:58:32.841
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_2004017_01

Start Time:	2004-017T00:02:32.840	Stop Time:	2004-017T23:58:34.278
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_2004018_01

Start Time:	2004-018T00:02:34.276	Stop Time:	2004-018T23:58:35.714
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_2004019_01

Start Time:	2004-019T00:02:35.712	Stop Time:	2004-019T23:58:37.150
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_2004020_01

Start Time:	2004-020T00:02:37.149	Stop Time:	2004-020T23:58:38.587
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004021_01

Start Time:	2004-021T00:02:38.585	Stop Time:	2004-021T23:58:41.022
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004022_01

Start Time:	2004-022T00:02:41.020	Stop Time:	2004-022T23:58:42.458
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004023_01

Start Time:	2004-023T00:02:42.457	Stop Time:	2004-023T23:58:43.895
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004024_01

Start Time:	2004-024T00:02:43.893	Stop Time:	2004-024T23:58:45.331
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004025_01

Start Time:	2004-025T00:02:45.329	Stop Time:	2004-025T23:58:46.767
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004026_01

Start Time:	2004-026T00:02:46.766	Stop Time:	2004-026T22:46:47.232
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004027_01

Start Time:	2004-027T00:26:49.193	Stop Time:	2004-027T23:58:50.640
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_2004028_01

Start Time:	2004-028T00:02:50.638	Stop Time:	2004-028T23:58:52.076
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_2004029_01

Start Time:	2004-029T00:02:52.075	Stop Time:	2004-029T23:58:53.513
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004030_01

Start Time:	2004-030T00:02:53.511	Stop Time:	2004-030T23:58:54.949
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004031_01

Start Time:	2004-031T00:02:54.947	Stop Time:	2004-031T23:58:57.385
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004032_01

Start Time:	2004-032T00:02:57.384	Stop Time:	2004-032T23:58:57.822
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004033_01

Start Time:	2004-033T00:02:57.820	Stop Time:	2004-033T23:59:00.258
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_2004034_01

Start Time:	2004-034T00:03:00.256	Stop Time:	2004-034T23:59:01.694
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_2004035_01

Start Time:	2004-035T00:03:01.693	Stop Time:	2004-035T23:59:03.131
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004036_01

Start Time:	2004-036T00:03:03.129	Stop Time:	2004-036T23:59:04.567
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004037_01

Start Time:	2004-037T00:03:04.565	Stop Time:	2004-037T23:59:06.003
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004038_01

Start Time:	2004-038T00:03:55.220	Stop Time:	2004-038T23:55:41.660
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004039_01

Start Time:	2004-039T00:01:26.658	Stop Time:	2004-039T23:58:57.095
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004040_01

Start Time:	2004-040T00:04:42.093	Stop Time:	2004-040T23:56:28.532
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004041_01

Start Time:	2004-041T00:02:13.530	Stop Time:	2004-041T23:59:44.967
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004042_01

Start Time:	2004-042T00:05:29.965	Stop Time:	2004-042T23:57:15.405
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004043_01

Start Time:	2004-043T00:03:00.402	Stop Time:	2004-043T23:54:46.842
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004044_01

Start Time:	2004-044T00:00:31.840	Stop Time:	2004-044T23:58:02.277
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_2004045_01

Start Time:	2004-045T00:03:47.275	Stop Time:	2004-045T23:55:33.714
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_2004046_01

Start Time:	2004-046T00:01:18.712	Stop Time:	2004-046T23:58:50.149
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_2004047_01

Start Time:	2004-047T00:04:35.147	Stop Time:	2004-047T23:56:20.587
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004048_01

Start Time:	2004-048T00:02:05.584	Stop Time:	2004-048T23:59:37.022
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004049_01

Start Time:	2004-049T00:05:22.019	Stop Time:	2004-049T23:57:08.459
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_2004050_01

Start Time:	2004-050T00:02:53.457	Stop Time:	2004-050T23:54:38.896
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004051_01

Start Time:	2004-051T00:00:22.894	Stop Time:	2004-051T23:59:11.237
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004052_01

Start Time:	2004-052T00:04:11.235	Stop Time:	2004-052T23:58:54.177
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_2004053_01

Start Time:	2004-053T00:03:16.176	Stop Time:	2004-053T23:58:18.110
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004054_01

Start Time:	2004-054T00:03:18.108	Stop Time:	2004-054T23:56:06.438
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004055_01

Start Time:	2004-055T00:00:26.624	Stop Time:	2004-055T23:59:29.982
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004056_01

Start Time:	2004-056T00:04:29.980	Stop Time:	2004-056T23:59:31.419
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_2004057_01

Start Time:	2004-057T00:04:31.417	Stop Time:	2004-057T23:59:31.855
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004058_01

Start Time:	2004-058T00:04:31.853	Stop Time:	2004-058T23:57:31.355
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004059_01

Start Time:	2004-059T00:03:01.352	Stop Time:	2004-059T23:58:31.791
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004060_01

Start Time:	2004-060T00:04:01.788	Stop Time:	2004-060T22:48:01.255
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004064_01

Start Time:	2004-064T23:05:49.993	Stop Time:	2004-064T23:55:49.911
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004065_01

Start Time:	2004-065T00:00:49.909	Stop Time:	2004-065T23:55:50.347
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004066_01

Start Time:	2004-066T00:00:50.345	Stop Time:	2004-066T23:57:51.673
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004067_01

Start Time:	2004-067T00:02:12.468	Stop Time:	2004-067T23:59:45.218
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004068_01

Start Time:	2004-068T00:04:45.216	Stop Time:	2004-068T23:58:35.138
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_2004069_01

Start Time:	2004-069T00:02:57.156	Stop Time:	2004-069T23:56:46.091
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_2004070_01

Start Time:	2004-070T00:01:46.089	Stop Time:	2004-070T23:56:46.527
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004071_01

Start Time:	2004-071T00:01:46.525	Stop Time:	2004-071T23:59:12.963
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004072_01

Start Time:	2004-072T00:04:12.961	Stop Time:	2004-072T23:59:14.399
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_2004073_01

Start Time:	2004-073T00:04:14.397	Stop Time:	2004-073T23:58:06.836
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_2004074_01

Start Time:	2004-074T00:03:06.834	Stop Time:	2004-074T23:58:07.272
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004075_01

Start Time:	2004-075T00:03:07.270	Stop Time:	2004-075T23:58:07.709
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_2004076_01

Start Time:	2004-076T00:03:07.707	Stop Time:	2004-076T23:58:39.145
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004077_01

Start Time:	2004-077T00:03:39.143	Stop Time:	2004-077T23:58:39.581
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_2004078_01

Start Time:	2004-078T00:03:39.579	Stop Time:	2004-078T23:55:54.018
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004079_01

Start Time:	2004-079T00:00:54.016	Stop Time:	2004-079T23:55:55.455
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_2004080_01

Start Time:	2004-080T00:00:55.453	Stop Time:	2004-080T16:15:55.071
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004081_01

Start Time:	2004-081T01:00:56.866	Stop Time:	2004-081T23:55:57.327
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004082_01

Start Time:	2004-082T00:00:57.325	Stop Time:	2004-082T23:55:42.518
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004083_01

Start Time:	2004-083T00:00:02.641	Stop Time:	2004-083T23:57:18.200
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004084_01

Start Time:	2004-084T00:02:18.198	Stop Time:	2004-084T23:57:19.636
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004085_01

Start Time:	2004-085T00:02:19.634	Stop Time:	2004-085T23:56:06.073
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004086_01

Start Time:	2004-086T00:01:06.071	Stop Time:	2004-086T23:56:07.509
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_2004087_01

Start Time:	2004-087T00:01:07.507	Stop Time:	2004-087T23:58:29.823
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004088_01

Start Time:	2004-088T00:02:49.630	Stop Time:	2004-088T23:58:01.425
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004089_01

Start Time:	2004-089T00:03:01.423	Stop Time:	2004-089T23:56:11.543
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_2004090_01

Start Time:	2004-090T00:00:32.752	Stop Time:	2004-090T23:59:30.362
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004091_01

Start Time:	2004-091T00:05:00.359	Stop Time:	2004-091T23:55:00.801
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004092_01

Start Time:	2004-092T00:00:30.798	Stop Time:	2004-092T23:56:01.050
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_2004093_01

Start Time:	2004-093T00:00:01.048	Stop Time:	2004-093T23:56:02.487
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004094_01

Start Time:	2004-094T00:00:02.486	Stop Time:	2004-094T23:56:04.925
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_2004095_01

Start Time:	2004-095T00:00:04.923	Stop Time:	2004-095T23:57:56.361
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_2004096_01

Start Time:	2004-096T00:01:56.360	Stop Time:	2004-096T23:59:46.610
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_2004097_01

Start Time:	2004-097T00:04:07.218	Stop Time:	2004-097T23:57:09.236
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004098_01

Start Time:	2004-098T00:01:09.234	Stop Time:	2004-098T23:57:10.673
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004099_01

Start Time:	2004-099T00:01:10.672	Stop Time:	2004-099T23:59:28.110
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004100_01

Start Time:	2004-100T00:03:28.108	Stop Time:	2004-100T23:55:57.954
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004101_01

Start Time:	2004-101T00:00:19.562	Stop Time:	2004-101T23:59:44.984
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004102_01

Start Time:	2004-102T00:03:44.982	Stop Time:	2004-102T23:59:46.421
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004103_01

Start Time:	2004-103T00:03:46.420	Stop Time:	2004-103T23:58:48.859
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004104_01

Start Time:	2004-104T00:02:48.857	Stop Time:	2004-104T23:59:46.296
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_2004105_01

Start Time:	2004-105T00:03:46.294	Stop Time:	2004-105T23:59:47.733
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_2004106_01

Start Time:	2004-106T00:03:47.732	Stop Time:	2004-106T23:59:50.170
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004107_01

Start Time:	2004-107T00:03:50.169	Stop Time:	2004-107T23:59:50.608
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004108_01

Start Time:	2004-108T00:03:50.606	Stop Time:	2004-108T23:58:34.881
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_2004109_01

Start Time:	2004-109T00:02:55.653	Stop Time:	2004-109T23:58:53.483
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004110_01

Start Time:	2004-110T00:02:53.481	Stop Time:	2004-110T23:59:58.669
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004111_01

Start Time:	2004-111T00:01:58.669	Stop Time:	2004-111T23:58:04.357
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_2004112_01

Start Time:	2004-112T00:02:04.356	Stop Time:	2004-112T23:59:44.216
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004113_01

Start Time:	2004-113T00:04:04.796	Stop Time:	2004-113T23:59:06.232
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004114_01

Start Time:	2004-114T00:03:06.230	Stop Time:	2004-114T23:59:07.669
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004115_01

Start Time:	2004-115T00:03:07.667	Stop Time:	2004-115T23:56:33.107
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_2004116_01

Start Time:	2004-116T00:00:33.105	Stop Time:	2004-116T23:57:45.559
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004117_01

Start Time:	2004-117T00:02:06.964	Stop Time:	2004-117T23:58:10.981
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004118_01

Start Time:	2004-118T00:02:10.979	Stop Time:	2004-118T23:58:12.418
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004119_01

Start Time:	2004-119T00:02:12.417	Stop Time:	2004-119T23:58:13.856
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004120_01

Start Time:	2004-120T00:02:13.854	Stop Time:	2004-120T23:58:16.294
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004121_01

Start Time:	2004-121T00:02:16.292	Stop Time:	2004-121T23:58:17.731
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_2004122_01

Start Time:	2004-122T00:02:17.729	Stop Time:	2004-122T23:58:19.168
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004123_01

Start Time:	2004-123T00:02:19.167	Stop Time:	2004-123T23:58:20.605
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004124_01

Start Time:	2004-124T00:02:20.604	Stop Time:	2004-124T23:57:50.043
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_2004125_01

Start Time:	2004-125T00:01:50.041	Stop Time:	2004-125T23:56:02.700
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_2004126_01

Start Time:	2004-126T00:00:24.698	Stop Time:	2004-126T23:59:56.917
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004127_01

Start Time:	2004-127T00:03:56.915	Stop Time:	2004-127T23:59:02.104
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_2004128_01

Start Time:	2004-128T00:01:02.103	Stop Time:	2004-128T23:59:19.791
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004129_01

Start Time:	2004-129T00:03:19.790	Stop Time:	2004-129T23:59:42.838
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004130_01

Start Time:	2004-130T00:04:02.242	Stop Time:	2004-130T23:58:55.666
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004131_01

Start Time:	2004-131T00:02:55.664	Stop Time:	2004-131T23:58:57.103
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004132_01

Start Time:	2004-132T00:02:57.102	Stop Time:	2004-132T23:59:05.290
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004133_01

Start Time:	2004-133T00:01:05.290	Stop Time:	2004-133T23:58:36.728
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_2004134_01

Start Time:	2004-134T00:00:36.727	Stop Time:	2004-134T23:57:18.416
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004135_01

Start Time:	2004-135T00:01:19.414	Stop Time:	2004-135T23:56:11.853
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004136_01

Start Time:	2004-136T00:00:11.852	Stop Time:	2004-136T23:56:13.291
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004137_01

Start Time:	2004-137T00:00:13.289	Stop Time:	2004-137T23:56:14.728
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_2004138_01

Start Time:	2004-138T00:00:14.726	Stop Time:	2004-138T23:56:16.165
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_2004139_01

Start Time:	2004-139T00:00:16.164	Stop Time:	2004-139T23:56:17.602
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_2004140_01

Start Time:	2004-140T00:00:17.601	Stop Time:	2004-140T23:56:20.040
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004141_01

Start Time:	2004-141T00:00:20.038	Stop Time:	2004-141T23:56:17.477
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004142_01

Start Time:	2004-142T00:00:17.475	Stop Time:	2004-142T23:56:03.524
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004143_01

Start Time:	2004-143T00:00:23.522	Stop Time:	2004-143T23:57:05.960
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004144_01

Start Time:	2004-144T00:01:29.185	Stop Time:	2004-144T23:57:01.788
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.

CMFULL0_2004145_01

Start Time:	2004-145T00:01:01.787	Stop Time:	2004-145T23:59:03.893
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004146_01

Start Time:	2004-146T00:03:25.852	Stop Time:	2004-146T23:59:28.084
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_2004147_01

Start Time:	2004-147T00:03:49.270	Stop Time:	2004-147T23:58:18.100
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004148_01

Start Time:	2004-148T00:02:18.098	Stop Time:	2004-148T23:58:57.537
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004149_01

Start Time:	2004-149T00:02:57.535	Stop Time:	2004-149T23:56:11.787
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_2004150_01

Start Time:	2004-150T00:00:32.602	Stop Time:	2004-150T23:57:19.412
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_2004151_01

Start Time:	2004-151T00:01:19.410	Stop Time:	2004-151T23:59:37.864
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004152_01

Start Time:	2004-152T00:03:57.651	Stop Time:	2004-152T23:59:56.328
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_2004153_01

Start Time:	2004-153T00:04:18.096	Stop Time:	2004-153T23:58:39.926
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004154_01

Start Time:	2004-154T00:03:00.924	Stop Time:	2004-154T23:55:52.380
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004155_01

Start Time:	2004-155T00:00:13.582	Stop Time:	2004-155T23:57:36.004
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_2004156_01

Start Time:	2004-156T00:01:59.018	Stop Time:	2004-156T23:58:15.035
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004157_01

Start Time:	2004-157T00:02:15.033	Stop Time:	2004-157T23:58:02.472
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004158_01

Start Time:	2004-158T00:02:02.471	Stop Time:	2004-158T23:58:05.913
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004159_01

Start Time:	2004-159T00:02:26.912	Stop Time:	2004-159T23:58:51.346
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004160_01

Start Time:	2004-160T00:02:51.345	Stop Time:	2004-160T23:55:45.207
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004161_01

Start Time:	2004-161T00:00:06.393	Stop Time:	2004-161T23:57:11.440
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004162_01

Start Time:	2004-162T00:01:30.825	Stop Time:	2004-162T23:56:26.464
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004163_01

Start Time:	2004-163T00:00:49.286	Stop Time:	2004-163T23:57:44.096
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004164_01

Start Time:	2004-164T00:01:44.094	Stop Time:	2004-164T23:59:31.532
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004165_01

Start Time:	2004-165T00:03:31.531	Stop Time:	2004-165T23:58:23.970
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_2004166_01

Start Time:	2004-166T00:02:23.969	Stop Time:	2004-166T23:59:25.407
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004167_01

Start Time:	2004-167T00:03:25.405	Stop Time:	2004-167T23:57:37.118
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004168_01

Start Time:	2004-168T00:03:35.116	Stop Time:	2004-168T23:58:19.283
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_2004169_01

Start Time:	2004-169T00:02:19.281	Stop Time:	2004-169T23:59:26.470
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004170_01

Start Time:	2004-170T00:01:26.469	Stop Time:	2004-170T23:58:52.907
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004171_01

Start Time:	2004-171T00:00:52.906	Stop Time:	2004-171T23:56:50.595
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004172_01

Start Time:	2004-172T00:00:50.594	Stop Time:	2004-172T23:56:48.032
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004173_01

Start Time:	2004-173T00:00:48.031	Stop Time:	2004-173T23:56:49.470
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004174_01

Start Time:	2004-174T00:00:49.468	Stop Time:	2004-174T23:56:50.907
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004175_01

Start Time:	2004-175T00:00:50.905	Stop Time:	2004-175T23:58:57.093
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_2004176_01

Start Time:	2004-176T00:00:57.093	Stop Time:	2004-176T23:58:57.531
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004177_01

Start Time:	2004-177T00:00:59.463	Stop Time:	2004-177T23:58:59.968
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004178_01

Start Time:	2004-178T00:00:59.967	Stop Time:	2004-178T23:59:01.405
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004179_01

Start Time:	2004-179T00:01:01.404	Stop Time:	2004-179T23:59:02.842
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004180_01

Start Time:	2004-180T00:01:02.842	Stop Time:	2004-180T23:59:04.280
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004181_01

Start Time:	2004-181T00:01:04.279	Stop Time:	2004-181T23:59:05.717
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_2004182_01

Start Time:	2004-182T00:01:05.716	Stop Time:	2004-182T23:59:07.154
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004183_01

Start Time:	2004-183T00:01:07.153	Stop Time:	2004-183T23:57:27.842
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004184_01

Start Time:	2004-184T00:01:27.840	Stop Time:	2004-184T23:57:29.279
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004185_01

Start Time:	2004-185T00:01:29.278	Stop Time:	2004-185T23:57:30.716
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_2004186_01

Start Time:	2004-186T00:01:30.715	Stop Time:	2004-186T05:17:29.591
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004194_01

Start Time:	2004-194T22:34:48.434	Stop Time:	2004-194T23:58:47.401
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004195_01

Start Time:	2004-195T00:00:47.400	Stop Time:	2004-195T23:58:49.838
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004196_01

Start Time:	2004-196T00:00:49.838	Stop Time:	2004-196T23:58:51.276
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_2004197_01

Start Time:	2004-197T00:00:51.275	Stop Time:	2004-197T23:59:04.713
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004198_01

Start Time:	2004-198T00:01:04.712	Stop Time:	2004-198T23:58:03.150
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_2004199_01

Start Time:	2004-199T00:00:03.150	Stop Time:	2004-199T23:58:04.588
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004200_01

Start Time:	2004-200T00:00:04.587	Stop Time:	2004-200T23:58:06.025
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004201_01

Start Time:	2004-201T00:00:06.024	Stop Time:	2004-201T23:59:48.461
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004202_01

Start Time:	2004-202T00:01:48.461	Stop Time:	2004-202T23:58:24.899
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004203_01

Start Time:	2004-203T00:00:24.898	Stop Time:	2004-203T23:58:08.337
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_2004204_01

Start Time:	2004-204T00:00:08.336	Stop Time:	2004-204T23:58:21.775
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_2004205_01

Start Time:	2004-205T00:00:21.774	Stop Time:	2004-205T23:59:56.211
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004206_01

Start Time:	2004-206T00:01:56.211	Stop Time:	2004-206T23:58:14.649
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004207_01

Start Time:	2004-207T00:00:14.649	Stop Time:	2004-207T23:58:23.086
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004208_01

Start Time:	2004-208T00:00:23.086	Stop Time:	2004-208T23:59:50.523
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004209_01

Start Time:	2004-209T00:01:50.522	Stop Time:	2004-209T23:58:39.961
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004210_01

Start Time:	2004-210T00:00:39.960	Stop Time:	2004-210T23:58:55.648
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_2004211_01

Start Time:	2004-211T00:02:55.646	Stop Time:	2004-211T23:58:57.085
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_2004212_01

Start Time:	2004-212T00:02:57.084	Stop Time:	2004-212T23:59:22.272
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004213_01

Start Time:	2004-213T00:01:22.272	Stop Time:	2004-213T23:59:42.709
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_2004214_01

Start Time:	2004-214T00:01:42.709	Stop Time:	2004-214T23:59:44.147
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004215_01

Start Time:	2004-215T00:01:44.146	Stop Time:	2004-215T23:59:46.584
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004216_01

Start Time:	2004-216T00:01:46.583	Stop Time:	2004-216T23:59:48.021
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_2004217_01

Start Time:	2004-217T00:01:48.020	Stop Time:	2004-217T23:59:49.458
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004218_01

Start Time:	2004-218T00:01:49.458	Stop Time:	2004-218T23:59:50.896
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004219_01

Start Time:	2004-219T00:01:50.895	Stop Time:	2004-219T23:56:22.584
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004220_01

Start Time:	2004-220T00:00:22.583	Stop Time:	2004-220T23:58:57.021
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_2004221_01

Start Time:	2004-221T00:02:57.019	Stop Time:	2004-221T23:58:42.458
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004222_01

Start Time:	2004-222T00:02:42.456	Stop Time:	2004-222T23:56:06.896
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004223_01

Start Time:	2004-223T00:00:06.895	Stop Time:	2004-223T23:59:21.332
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_2004224_01

Start Time:	2004-224T00:03:21.331	Stop Time:	2004-224T23:59:34.769
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004225_01

Start Time:	2004-225T00:03:34.768	Stop Time:	2004-225T23:58:02.207
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004226_01

Start Time:	2004-226T00:02:02.206	Stop Time:	2004-226T23:56:12.645
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004227_01

Start Time:	2004-227T00:00:12.644	Stop Time:	2004-227T23:56:31.082
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_2004228_01

Start Time:	2004-228T00:00:31.081	Stop Time:	2004-228T23:56:46.519
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_2004229_01

Start Time:	2004-229T00:00:46.518	Stop Time:	2004-229T23:57:33.956
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_2004230_01

Start Time:	2004-230T00:01:33.955	Stop Time:	2004-230T23:59:14.393
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004231_01

Start Time:	2004-231T00:03:14.391	Stop Time:	2004-231T23:56:13.831
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_2004232_01

Start Time:	2004-232T00:00:13.830	Stop Time:	2004-232T23:58:19.268
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_2004233_01

Start Time:	2004-233T00:02:19.266	Stop Time:	2004-233T23:56:59.706
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004234_01

Start Time:	2004-234T00:00:59.704	Stop Time:	2004-234T23:58:23.142
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004235_01

Start Time:	2004-235T00:02:23.141	Stop Time:	2004-235T23:59:39.579
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_2004236_01

Start Time:	2004-236T00:03:39.577	Stop Time:	2004-236T23:59:41.016
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004237_01

Start Time:	2004-237T00:03:41.015	Stop Time:	2004-237T23:59:42.454
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004238_01

Start Time:	2004-238T00:03:42.452	Stop Time:	2004-238T23:57:16.892
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004239_01

Start Time:	2004-239T00:01:16.890	Stop Time:	2004-239T23:58:55.328
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_2004240_01

Start Time:	2004-240T00:02:55.327	Stop Time:	2004-240T23:56:41.766
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_2004241_01

Start Time:	2004-241T00:00:41.765	Stop Time:	2004-241T23:58:16.203
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004242_01

Start Time:	2004-242T00:02:16.202	Stop Time:	2004-242T23:59:03.640
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_2004243_01

Start Time:	2004-243T00:03:03.639	Stop Time:	2004-243T23:59:05.077
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004244_01

Start Time:	2004-244T00:03:05.076	Stop Time:	2004-244T23:57:55.515
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004245_01

Start Time:	2004-245T00:01:55.513	Stop Time:	2004-245T23:59:03.952
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004246_01

Start Time:	2004-246T00:03:03.950	Stop Time:	2004-246T23:59:49.389
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004247_01

Start Time:	2004-247T00:03:49.387	Stop Time:	2004-247T23:58:32.827
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_2004248_01

Start Time:	2004-248T00:02:32.825	Stop Time:	2004-248T23:58:34.264
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004249_01

Start Time:	2004-249T00:02:34.262	Stop Time:	2004-249T23:57:00.702
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004250_01

Start Time:	2004-250T00:01:00.700	Stop Time:	2004-250T23:56:32.139
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004251_01

Start Time:	2004-251T00:00:32.138	Stop Time:	2004-251T23:56:33.576
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004252_01

Start Time:	2004-252T00:00:33.575	Stop Time:	2004-252T23:56:35.014
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004253_01

Start Time:	2004-253T00:00:35.012	Stop Time:	2004-253T23:58:55.451
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004254_01

Start Time:	2004-254T00:02:55.449	Stop Time:	2004-254T23:58:56.888
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_2004255_01

Start Time:	2004-255T00:02:56.887	Stop Time:	2004-255T23:57:51.326
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004256_01

Start Time:	2004-256T00:01:51.324	Stop Time:	2004-256T23:59:17.763
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004257_01

Start Time:	2004-257T00:03:17.761	Stop Time:	2004-257T23:59:19.200
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004258_01

Start Time:	2004-258T00:03:19.198	Stop Time:	2004-258T23:59:20.637
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_2004259_01

Start Time:	2004-259T00:03:20.636	Stop Time:	2004-259T23:56:02.076
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_2004260_01

Start Time:	2004-260T00:00:02.074	Stop Time:	2004-260T23:58:46.512
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004261_01

Start Time:	2004-261T00:02:46.510	Stop Time:	2004-261T23:56:52.950
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_2004262_01

Start Time:	2004-262T00:00:52.948	Stop Time:	2004-262T23:56:54.387
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004263_01

Start Time:	2004-263T00:00:54.386	Stop Time:	2004-263T23:56:55.824
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_2004264_01

Start Time:	2004-264T00:00:55.823	Stop Time:	2004-264T23:56:58.262
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_2004265_01

Start Time:	2004-265T00:00:58.260	Stop Time:	2004-265T23:57:12.699
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004266_01

Start Time:	2004-266T00:01:12.697	Stop Time:	2004-266T23:57:14.136
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004267_01

Start Time:	2004-267T00:01:14.135	Stop Time:	2004-267T23:59:58.572
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004268_01

Start Time:	2004-268T00:03:58.571	Stop Time:	2004-268T23:56:45.011
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004269_01

Start Time:	2004-269T00:00:45.009	Stop Time:	2004-269T23:56:46.448
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004270_01

Start Time:	2004-270T00:00:46.447	Stop Time:	2004-270T23:56:47.885
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004271_01

Start Time:	2004-271T00:00:47.884	Stop Time:	2004-271T23:57:09.323
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004272_01

Start Time:	2004-272T00:01:09.321	Stop Time:	2004-272T23:58:15.759
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004273_01

Start Time:	2004-273T00:02:15.758	Stop Time:	2004-273T23:59:25.196
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004274_01

Start Time:	2004-274T00:03:25.195	Stop Time:	2004-274T23:57:49.634
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004275_01

Start Time:	2004-275T00:01:49.633	Stop Time:	2004-275T23:56:28.072
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004276_01

Start Time:	2004-276T00:00:28.070	Stop Time:	2004-276T23:56:29.509
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_2004277_01

Start Time:	2004-277T00:00:28.508	Stop Time:	2004-277T23:56:30.946
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_2004278_01

Start Time:	2004-278T00:00:30.945	Stop Time:	2004-278T23:56:32.384
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_2004279_01

Start Time:	2004-279T00:00:32.382	Stop Time:	2004-279T23:56:33.781
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_2004280_01

Start Time:	2004-280T00:00:33.779	Stop Time:	2004-280T23:56:35.217
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_2004281_01

Start Time:	2004-281T00:00:35.216	Stop Time:	2004-281T23:59:06.652
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_2004282_01

Start Time:	2004-282T00:03:06.651	Stop Time:	2004-282T23:58:04.089
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004283_01

Start Time:	2004-283T00:02:04.087	Stop Time:	2004-283T23:58:35.525
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004284_01

Start Time:	2004-284T00:02:35.523	Stop Time:	2004-284T23:58:36.961
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004285_01

Start Time:	2004-285T00:02:36.959	Stop Time:	2004-285T23:58:44.397
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_2004286_01

Start Time:	2004-286T00:02:44.395	Stop Time:	2004-286T23:58:51.833
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_2004287_01

Start Time:	2004-287T00:02:51.832	Stop Time:	2004-287T23:58:53.269
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004288_01

Start Time:	2004-288T00:02:53.268	Stop Time:	2004-288T23:58:46.706
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004289_01

Start Time:	2004-289T00:02:46.704	Stop Time:	2004-289T23:56:49.142
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004290_01

Start Time:	2004-290T00:00:49.141	Stop Time:	2004-290T23:58:14.578
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004291_01

Start Time:	2004-291T00:02:14.576	Stop Time:	2004-291T23:56:51.015
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004292_01

Start Time:	2004-292T00:00:51.013	Stop Time:	2004-292T23:57:07.451
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004293_01

Start Time:	2004-293T00:01:07.449	Stop Time:	2004-293T23:57:07.887
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_2004294_01

Start Time:	2004-294T00:01:07.885	Stop Time:	2004-294T23:56:50.323
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004295_01

Start Time:	2004-295T00:00:50.322	Stop Time:	2004-295T23:59:39.758
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004296_01

Start Time:	2004-296T00:03:39.757	Stop Time:	2004-296T23:59:44.944
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_2004297_01

Start Time:	2004-297T00:01:44.944	Stop Time:	2004-297T23:59:46.381
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_2004298_01

Start Time:	2004-298T00:01:46.380	Stop Time:	2004-298T23:59:12.067
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_2004299_01

Start Time:	2004-299T00:03:12.065	Stop Time:	2004-299T23:59:13.503
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004300_01

Start Time:	2004-300T00:03:13.502	Stop Time:	2004-300T23:56:49.940
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_2004301_01

Start Time:	2004-301T00:00:49.939	Stop Time:	2004-301T23:59:55.125
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004302_01

Start Time:	2004-302T00:02:51.374	Stop Time:	2004-302T23:58:56.562
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004303_01

Start Time:	2004-303T00:00:56.561	Stop Time:	2004-303T23:58:56.248
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004304_01

Start Time:	2004-304T00:02:56.246	Stop Time:	2004-304T23:58:02.433
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004305_01

Start Time:	2004-305T00:00:02.433	Stop Time:	2004-305T23:59:35.869
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004306_01

Start Time:	2004-306T00:01:35.868	Stop Time:	2004-306T23:58:40.306
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_2004307_01

Start Time:	2004-307T00:00:40.305	Stop Time:	2004-307T23:59:57.741
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004308_01

Start Time:	2004-308T00:01:57.740	Stop Time:	2004-308T23:59:17.178
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_2004309_01

Start Time:	2004-309T00:01:17.177	Stop Time:	2004-309T23:59:32.547
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004310_01

Start Time:	2004-310T00:01:32.613	Stop Time:	2004-310T23:59:33.050
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_2004311_01

Start Time:	2004-311T00:01:33.049	Stop Time:	2004-311T23:59:40.486
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004312_01

Start Time:	2004-312T00:01:40.485	Stop Time:	2004-312T23:58:18.923
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004313_01

Start Time:	2004-313T00:00:18.922	Stop Time:	2004-313T23:58:20.359
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004314_01

Start Time:	2004-314T00:00:20.358	Stop Time:	2004-314T23:58:21.795
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004315_01

Start Time:	2004-315T00:00:21.794	Stop Time:	2004-315T23:56:14.091
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_2004316_01

Start Time:	2004-316T00:00:35.699	Stop Time:	2004-316T23:59:50.667
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_2004317_01

Start Time:	2004-317T00:01:50.666	Stop Time:	2004-317T23:59:28.103
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004318_01

Start Time:	2004-318T00:01:28.102	Stop Time:	2004-318T23:59:29.539
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004319_01

Start Time:	2004-319T00:01:29.539	Stop Time:	2004-319T23:59:53.229
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_2004320_01

Start Time:	2004-320T00:04:13.228	Stop Time:	2004-320T23:58:34.412
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_2004321_01

Start Time:	2004-321T00:00:34.411	Stop Time:	2004-321T23:59:01.848
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_2004322_01

Start Time:	2004-322T00:01:01.847	Stop Time:	2004-322T23:58:40.202
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004323_01

Start Time:	2004-323T00:03:02.369	Stop Time:	2004-323T23:59:14.720
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004324_01

Start Time:	2004-324T00:01:14.719	Stop Time:	2004-324T23:58:52.157
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004325_01

Start Time:	2004-325T00:00:52.156	Stop Time:	2004-325T23:58:06.593
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_2004326_01

Start Time:	2004-326T00:00:06.592	Stop Time:	2004-326T23:59:28.115
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004327_01

Start Time:	2004-327T00:03:48.683	Stop Time:	2004-327T23:59:59.465
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004328_01

Start Time:	2004-328T00:01:59.464	Stop Time:	2004-328T23:58:00.902
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004329_01

Start Time:	2004-329T00:00:00.901	Stop Time:	2004-329T23:58:02.338
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_2004330_01

Start Time:	2004-330T00:00:02.337	Stop Time:	2004-330T23:59:14.774
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004331_01

Start Time:	2004-331T00:01:14.773	Stop Time:	2004-331T23:59:16.210
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004332_01

Start Time:	2004-332T00:01:16.209	Stop Time:	2004-332T23:59:55.646
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004333_01

Start Time:	2004-333T00:01:55.645	Stop Time:	2004-333T23:59:58.138
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_2004334_01

Start Time:	2004-334T00:01:58.137	Stop Time:	2004-334T23:59:59.575
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004335_01

Start Time:	2004-335T00:01:59.575	Stop Time:	2004-335T23:58:01.014
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004336_01

Start Time:	2004-336T00:00:01.013	Stop Time:	2004-336T23:58:02.451
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004337_01

Start Time:	2004-337T00:00:02.450	Stop Time:	2004-337T23:58:04.888
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_2004338_01

Start Time:	2004-338T00:00:04.888	Stop Time:	2004-338T23:58:06.326
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004339_01

Start Time:	2004-339T00:00:06.325	Stop Time:	2004-339T23:58:07.763
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004340_01

Start Time:	2004-340T00:00:07.763	Stop Time:	2004-340T23:58:09.201
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_2004341_01

Start Time:	2004-341T00:00:09.200	Stop Time:	2004-341T23:58:10.638
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004342_01

Start Time:	2004-342T00:00:10.638	Stop Time:	2004-342T23:59:56.544
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004343_01

Start Time:	2004-343T00:04:20.991	Stop Time:	2004-343T23:59:48.184
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_2004344_01

Start Time:	2004-344T00:04:10.370	Stop Time:	2004-344T23:59:29.950
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_2004345_01

Start Time:	2004-345T00:01:29.949	Stop Time:	2004-345T23:59:31.388
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004346_01

Start Time:	2004-346T00:01:31.387	Stop Time:	2004-346T23:59:32.825
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004347_01

Start Time:	2004-347T00:01:32.824	Stop Time:	2004-347T23:57:30.513
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004348_01

Start Time:	2004-348T00:01:30.512	Stop Time:	2004-348T23:59:24.153
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004349_01

Start Time:	2004-349T00:03:46.991	Stop Time:	2004-349T23:58:12.388
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004350_01

Start Time:	2004-350T00:02:12.386	Stop Time:	2004-350T23:59:21.825
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004351_01

Start Time:	2004-351T00:03:21.824	Stop Time:	2004-351T23:59:23.262
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_2004352_01

Start Time:	2004-352T00:02:27.010	Stop Time:	2004-352T23:58:29.449
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004353_01

Start Time:	2004-353T00:00:29.449	Stop Time:	2004-353T23:58:30.887
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_2004354_01

Start Time:	2004-354T00:00:30.886	Stop Time:	2004-354T23:58:32.324
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004355_01

Start Time:	2004-355T00:00:32.324	Stop Time:	2004-355T23:58:33.762
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004356_01

Start Time:	2004-356T00:00:33.761	Stop Time:	2004-356T23:58:35.199
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004357_01

Start Time:	2004-357T00:00:35.198	Stop Time:	2004-357T23:58:37.637
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_2004358_01

Start Time:	2004-358T00:00:37.636	Stop Time:	2004-358T23:58:39.074
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004359_01

Start Time:	2004-359T00:00:39.073	Stop Time:	2004-359T23:55:03.036
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004360_01

Start Time:	2004-360T00:01:00.034	Stop Time:	2004-360T23:59:07.949
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004361_01

Start Time:	2004-361T00:01:07.948	Stop Time:	2004-361T23:59:10.386
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004362_01

Start Time:	2004-362T00:01:10.386	Stop Time:	2004-362T23:57:58.348
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004363_01

Start Time:	2004-363T00:03:56.345	Stop Time:	2004-363T23:59:57.261
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004364_01

Start Time:	2004-364T00:01:57.260	Stop Time:	2004-364T23:59:59.698
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004365_01

Start Time:	2004-365T00:01:59.698	Stop Time:	2004-365T23:56:57.387
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2004366_01

Start Time:	2004-366T00:00:57.386	Stop Time:	2004-366T23:56:24.825
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included 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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