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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/ 2005 /

CMFULL0_2005001_01

Start Time:	2005-001T00:00:24.823	Stop Time:	2005-001T23:56:26.262
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_2005002_01

Start Time:	2005-002T00:00:26.261	Stop Time:	2005-002T23:59:31.449
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_2005003_01

Start Time:	2005-003T00:01:31.448	Stop Time:	2005-003T23:59:32.886
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005004_01

Start Time:	2005-004T00:01:32.885	Stop Time:	2005-004T23:59:35.323
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_2005005_01

Start Time:	2005-005T00:01:35.323	Stop Time:	2005-005T23:59:36.761
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005006_01

Start Time:	2005-006T00:01:36.760	Stop Time:	2005-006T11:39:37.487
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_2005015_01

Start Time:	2005-015T16:51:22.553	Stop Time:	2005-015T23:59:22.386
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_2005016_01

Start Time:	2005-016T00:03:22.384	Stop Time:	2005-016T23:56:11.824
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_2005017_01

Start Time:	2005-017T00:00:11.823	Stop Time:	2005-017T23:59:17.011
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_2005018_01

Start Time:	2005-018T00:01:17.010	Stop Time:	2005-018T23:58:38.448
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_2005019_01

Start Time:	2005-019T00:00:38.448	Stop Time:	2005-019T23:59:30.886
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005020_01

Start Time:	2005-020T00:01:31.885	Stop Time:	2005-020T23:58:08.323
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_2005021_01

Start Time:	2005-021T00:00:08.322	Stop Time:	2005-021T23:59:10.760
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005022_01

Start Time:	2005-022T00:01:10.759	Stop Time:	2005-022T23:56:39.108
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005023_01

Start Time:	2005-023T00:00:01.591	Stop Time:	2005-023T23:59:18.635
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005024_01

Start Time:	2005-024T00:01:18.634	Stop Time:	2005-024T23:58:18.072
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_2005025_01

Start Time:	2005-025T00:00:18.072	Stop Time:	2005-025T23:58:19.510
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005026_01

Start Time:	2005-026T00:00:19.509	Stop Time:	2005-026T23:59:23.947
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005027_01

Start Time:	2005-027T00:01:23.946	Stop Time:	2005-027T23:59:21.384
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_2005028_01

Start Time:	2005-028T00:01:21.384	Stop Time:	2005-028T23:56:22.347
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_2005029_01

Start Time:	2005-029T00:02:20.344	Stop Time:	2005-029T23:58:13.408
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005030_01

Start Time:	2005-030T00:01:35.407	Stop Time:	2005-030T23:58:49.845
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005031_01

Start Time:	2005-031T00:02:11.579	Stop Time:	2005-031T23:58:59.134
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005032_01

Start Time:	2005-032T00:01:00.134	Stop Time:	2005-032T23:58:52.572
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_2005033_01

Start Time:	2005-033T00:01:30.481	Stop Time:	2005-033T23:58:08.010
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005034_01

Start Time:	2005-034T00:00:47.388	Stop Time:	2005-034T23:58:16.381
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_2005035_01

Start Time:	2005-035T00:00:15.446	Stop Time:	2005-035T23:57:37.397
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_2005036_01

Start Time:	2005-036T00:00:59.887	Stop Time:	2005-036T23:58:46.322
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005037_01

Start Time:	2005-037T00:00:46.321	Stop Time:	2005-037T23:58:54.763
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_2005038_01

Start Time:	2005-038T00:02:15.641	Stop Time:	2005-038T23:59:09.197
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005039_01

Start Time:	2005-039T00:01:09.196	Stop Time:	2005-039T23:58:27.634
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_2005040_01

Start Time:	2005-040T00:00:27.634	Stop Time:	2005-040T23:58:56.072
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_2005041_01

Start Time:	2005-041T00:00:56.071	Stop Time:	2005-041T23:57:36.639
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005042_01

Start Time:	2005-042T00:00:57.778	Stop Time:	2005-042T23:58:17.947
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005043_01

Start Time:	2005-043T00:00:17.946	Stop Time:	2005-043T23:59:06.021
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_2005044_01

Start Time:	2005-044T00:02:28.141	Stop Time:	2005-044T23:59:02.822
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_2005045_01

Start Time:	2005-045T00:01:02.821	Stop Time:	2005-045T23:59:53.259
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005046_01

Start Time:	2005-046T00:01:53.258	Stop Time:	2005-046T23:59:55.696
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005047_01

Start Time:	2005-047T00:01:55.695	Stop Time:	2005-047T23:58:56.134
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005048_01

Start Time:	2005-048T00:00:58.067	Stop Time:	2005-048T23:57:25.697
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005049_01

Start Time:	2005-049T00:00:25.696	Stop Time:	2005-049T23:57:26.134
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005050_01

Start Time:	2005-050T00:00:26.133	Stop Time:	2005-050T23:57:26.572
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_2005051_01

Start Time:	2005-051T00:00:26.571	Stop Time:	2005-051T23:58:53.009
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005052_01

Start Time:	2005-052T00:02:03.277	Stop Time:	2005-052T23:58:13.447
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005053_01

Start Time:	2005-053T00:01:13.445	Stop Time:	2005-053T23:58:12.884
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005054_01

Start Time:	2005-054T00:01:12.883	Stop Time:	2005-054T23:57:34.345
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005055_01

Start Time:	2005-055T00:00:58.445	Stop Time:	2005-055T23:58:15.544
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_2005056_01

Start Time:	2005-056T00:01:37.781	Stop Time:	2005-056T23:56:56.955
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005057_01

Start Time:	2005-057T00:00:18.098	Stop Time:	2005-057T23:59:32.525
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_2005058_01

Start Time:	2005-058T00:01:32.537	Stop Time:	2005-058T23:57:12.337
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_2005059_01

Start Time:	2005-059T00:00:33.578	Stop Time:	2005-059T23:59:29.647
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005060_01

Start Time:	2005-060T00:02:29.646	Stop Time:	2005-060T23:58:05.103
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_2005061_01

Start Time:	2005-061T00:01:05.102	Stop Time:	2005-061T23:58:13.102
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005062_01

Start Time:	2005-062T00:01:35.315	Stop Time:	2005-062T23:58:15.934
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005063_01

Start Time:	2005-063T00:01:15.933	Stop Time:	2005-063T23:04:15.399
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_2005064_01

Start Time:	2005-064T04:06:30.548	Stop Time:	2005-064T23:59:53.092
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005065_01

Start Time:	2005-065T00:03:14.454	Stop Time:	2005-065T23:57:37.393
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_2005066_01

Start Time:	2005-066T00:00:58.052	Stop Time:	2005-066T23:59:19.711
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005067_01

Start Time:	2005-067T00:02:19.710	Stop Time:	2005-067T23:59:16.031
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005068_01

Start Time:	2005-068T00:01:16.030	Stop Time:	2005-068T23:59:45.599
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005069_01

Start Time:	2005-069T00:02:45.598	Stop Time:	2005-069T23:58:02.919
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005070_01

Start Time:	2005-070T00:00:02.919	Stop Time:	2005-070T23:58:04.364
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005071_01

Start Time:	2005-071T00:00:04.363	Stop Time:	2005-071T23:58:57.933
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005072_01

Start Time:	2005-072T00:01:57.932	Stop Time:	2005-072T23:58:58.377
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005073_01

Start Time:	2005-073T00:01:58.376	Stop Time:	2005-073T23:58:58.822
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_2005074_01

Start Time:	2005-074T00:01:58.821	Stop Time:	2005-074T23:55:20.666
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_2005075_01

Start Time:	2005-075T00:01:18.664	Stop Time:	2005-075T23:58:39.734
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005076_01

Start Time:	2005-076T00:02:00.979	Stop Time:	2005-076T23:58:10.941
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005077_01

Start Time:	2005-077T00:01:32.939	Stop Time:	2005-077T23:59:29.232
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_2005078_01

Start Time:	2005-078T00:02:50.985	Stop Time:	2005-078T23:58:28.919
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005079_01

Start Time:	2005-079T00:00:28.919	Stop Time:	2005-079T23:58:30.364
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005080_01

Start Time:	2005-080T00:00:30.363	Stop Time:	2005-080T23:58:37.445
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005081_01

Start Time:	2005-081T00:01:59.201	Stop Time:	2005-081T23:59:35.764
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005082_01

Start Time:	2005-082T00:02:57.399	Stop Time:	2005-082T23:59:04.486
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_2005083_01

Start Time:	2005-083T00:02:25.606	Stop Time:	2005-083T23:56:43.779
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005084_01

Start Time:	2005-084T00:00:05.778	Stop Time:	2005-084T23:58:55.734
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005085_01

Start Time:	2005-085T00:02:18.713	Stop Time:	2005-085T23:58:42.667
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_2005086_01

Start Time:	2005-086T00:02:04.177	Stop Time:	2005-086T23:58:44.502
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005087_01

Start Time:	2005-087T00:02:05.985	Stop Time:	2005-087T23:57:13.045
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005088_01

Start Time:	2005-088T00:00:13.044	Stop Time:	2005-088T23:59:16.360
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005089_01

Start Time:	2005-089T00:01:15.363	Stop Time:	2005-089T23:58:44.933
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005090_01

Start Time:	2005-090T00:01:44.932	Stop Time:	2005-090T23:59:17.252
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005091_01

Start Time:	2005-091T00:01:17.252	Stop Time:	2005-091T23:59:18.697
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005092_01

Start Time:	2005-092T00:01:18.696	Stop Time:	2005-092T23:59:03.290
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_2005093_01

Start Time:	2005-093T00:02:26.023	Stop Time:	2005-093T23:59:48.585
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005094_01

Start Time:	2005-094T00:01:48.585	Stop Time:	2005-094T23:58:10.031
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005095_01

Start Time:	2005-095T00:00:10.030	Stop Time:	2005-095T23:58:31.623
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005096_01

Start Time:	2005-096T00:01:53.020	Stop Time:	2005-096T23:59:13.556
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005097_01

Start Time:	2005-097T00:02:34.945	Stop Time:	2005-097T23:59:00.121
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005098_01

Start Time:	2005-098T00:02:20.874	Stop Time:	2005-098T23:58:58.808
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005099_01

Start Time:	2005-099T00:00:58.807	Stop Time:	2005-099T23:59:00.252
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005100_01

Start Time:	2005-100T00:01:00.252	Stop Time:	2005-100T23:56:44.522
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005101_01

Start Time:	2005-101T00:00:07.158	Stop Time:	2005-101T23:59:45.604
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005102_01

Start Time:	2005-102T00:03:06.845	Stop Time:	2005-102T23:57:08.536
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005103_01

Start Time:	2005-103T00:01:30.124	Stop Time:	2005-103T23:58:14.649
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_2005104_01

Start Time:	2005-104T00:01:36.250	Stop Time:	2005-104T23:57:40.674
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005105_01

Start Time:	2005-105T00:00:40.673	Stop Time:	2005-105T23:59:07.995
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005106_01

Start Time:	2005-106T00:01:07.994	Stop Time:	2005-106T23:59:15.441
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005107_01

Start Time:	2005-107T00:01:15.440	Stop Time:	2005-107T23:58:23.012
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005108_01

Start Time:	2005-108T00:01:23.011	Stop Time:	2005-108T23:58:42.970
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_2005109_01

Start Time:	2005-109T00:02:03.242	Stop Time:	2005-109T23:57:34.905
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005110_01

Start Time:	2005-110T00:00:34.904	Stop Time:	2005-110T23:59:39.351
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005111_01

Start Time:	2005-111T00:02:39.350	Stop Time:	2005-111T23:59:51.672
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005112_01

Start Time:	2005-112T00:01:51.671	Stop Time:	2005-112T23:58:57.119
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005113_01

Start Time:	2005-113T00:00:57.118	Stop Time:	2005-113T23:58:56.690
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005114_01

Start Time:	2005-114T00:01:56.689	Stop Time:	2005-114T23:57:33.894
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005115_01

Start Time:	2005-115T00:00:55.768	Stop Time:	2005-115T23:57:09.337
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_2005116_01

Start Time:	2005-116T00:01:31.335	Stop Time:	2005-116T23:59:17.661
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005117_01

Start Time:	2005-117T00:02:40.660	Stop Time:	2005-117T23:58:57.619
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005118_01

Start Time:	2005-118T00:02:19.497	Stop Time:	2005-118T23:57:55.308
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005119_01

Start Time:	2005-119T00:01:23.967	Stop Time:	2005-119T23:57:17.369
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005120_01

Start Time:	2005-120T00:00:17.368	Stop Time:	2005-120T23:57:17.815
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005121_01

Start Time:	2005-121T00:00:17.814	Stop Time:	2005-121T23:59:22.261
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_2005122_01

Start Time:	2005-122T00:02:22.260	Stop Time:	2005-122T23:57:41.708
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005123_01

Start Time:	2005-123T00:00:41.706	Stop Time:	2005-123T23:58:15.029
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005124_01

Start Time:	2005-124T00:00:15.028	Stop Time:	2005-124T23:58:07.475
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005125_01

Start Time:	2005-125T00:00:07.474	Stop Time:	2005-125T23:58:46.831
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_2005126_01

Start Time:	2005-126T00:02:08.802	Stop Time:	2005-126T23:58:20.492
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005127_01

Start Time:	2005-127T00:01:20.491	Stop Time:	2005-127T23:56:27.724
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005128_01

Start Time:	2005-128T00:00:10.149	Stop Time:	2005-128T23:58:05.529
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005129_01

Start Time:	2005-129T00:01:27.653	Stop Time:	2005-129T23:58:30.976
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005130_01

Start Time:	2005-130T00:01:51.974	Stop Time:	2005-130T23:59:54.277
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_2005131_01

Start Time:	2005-131T00:02:54.276	Stop Time:	2005-131T23:59:54.723
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005132_01

Start Time:	2005-132T00:02:54.722	Stop Time:	2005-132T23:59:55.169
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005133_01

Start Time:	2005-133T00:02:55.168	Stop Time:	2005-133T23:59:55.616
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005134_01

Start Time:	2005-134T00:02:55.614	Stop Time:	2005-134T23:59:26.312
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005135_01

Start Time:	2005-135T00:02:48.065	Stop Time:	2005-135T23:58:48.383
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005136_01

Start Time:	2005-136T00:00:48.383	Stop Time:	2005-136T23:56:59.979
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005137_01

Start Time:	2005-137T00:00:22.099	Stop Time:	2005-137T23:58:11.276
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_2005138_01

Start Time:	2005-138T00:00:11.275	Stop Time:	2005-138T23:59:24.245
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005139_01

Start Time:	2005-139T00:05:22.243	Stop Time:	2005-139T23:58:29.294
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_2005140_01

Start Time:	2005-140T00:01:29.292	Stop Time:	2005-140T23:58:29.740
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005141_01

Start Time:	2005-141T00:01:29.739	Stop Time:	2005-141T23:59:00.186
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005142_01

Start Time:	2005-142T00:02:00.185	Stop Time:	2005-142T23:59:00.632
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005143_01

Start Time:	2005-143T00:02:00.631	Stop Time:	2005-143T23:59:08.981
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_2005144_01

Start Time:	2005-144T00:02:30.589	Stop Time:	2005-144T23:58:38.525
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_2005145_01

Start Time:	2005-145T00:01:38.524	Stop Time:	2005-145T23:58:56.846
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005146_01

Start Time:	2005-146T00:00:56.845	Stop Time:	2005-146T23:58:58.292
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005147_01

Start Time:	2005-147T00:00:58.291	Stop Time:	2005-147T23:58:02.739
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005148_01

Start Time:	2005-148T00:00:02.738	Stop Time:	2005-148T23:59:31.309
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005149_01

Start Time:	2005-149T00:02:31.308	Stop Time:	2005-149T23:57:44.026
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005150_01

Start Time:	2005-150T00:01:06.025	Stop Time:	2005-150T23:57:18.988
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005151_01

Start Time:	2005-151T00:00:40.225	Stop Time:	2005-151T23:59:57.094
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005152_01

Start Time:	2005-152T00:03:19.585	Stop Time:	2005-152T23:58:26.790
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005153_01

Start Time:	2005-153T00:01:48.789	Stop Time:	2005-153T23:57:55.240
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005154_01

Start Time:	2005-154T00:01:16.750	Stop Time:	2005-154T23:58:59.079
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005155_01

Start Time:	2005-155T00:02:21.430	Stop Time:	2005-155T23:58:50.505
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005156_01

Start Time:	2005-156T00:01:50.504	Stop Time:	2005-156T23:58:50.954
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_2005157_01

Start Time:	2005-157T00:01:50.953	Stop Time:	2005-157T23:56:49.549
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005158_01

Start Time:	2005-158T00:00:11.915	Stop Time:	2005-158T23:57:09.854
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005159_01

Start Time:	2005-159T00:00:09.852	Stop Time:	2005-159T23:59:10.302
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005160_01

Start Time:	2005-160T00:02:10.301	Stop Time:	2005-160T23:59:04.751
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005161_01

Start Time:	2005-161T00:02:04.750	Stop Time:	2005-161T23:58:51.201
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_2005162_01

Start Time:	2005-162T00:01:51.200	Stop Time:	2005-162T23:59:46.525
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_2005163_01

Start Time:	2005-163T00:01:46.524	Stop Time:	2005-163T23:57:47.979
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005164_01

Start Time:	2005-164T00:01:09.368	Stop Time:	2005-164T23:58:58.549
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005165_01

Start Time:	2005-165T00:01:58.547	Stop Time:	2005-165T23:58:06.385
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_2005166_01

Start Time:	2005-166T00:01:29.001	Stop Time:	2005-166T23:58:41.447
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005167_01

Start Time:	2005-167T00:01:41.446	Stop Time:	2005-167T23:59:29.440
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_2005168_01

Start Time:	2005-168T00:02:50.529	Stop Time:	2005-168T23:57:00.347
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_2005169_01

Start Time:	2005-169T00:00:00.346	Stop Time:	2005-169T23:59:53.796
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005170_01

Start Time:	2005-170T00:02:53.794	Stop Time:	2005-170T23:59:50.245
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005171_01

Start Time:	2005-171T00:02:50.244	Stop Time:	2005-171T23:56:40.480
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_2005172_01

Start Time:	2005-172T00:00:02.206	Stop Time:	2005-172T23:58:05.144
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005173_01

Start Time:	2005-173T00:01:05.143	Stop Time:	2005-173T23:56:52.980
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005174_01

Start Time:	2005-174T00:00:14.979	Stop Time:	2005-174T23:59:35.042
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005175_01

Start Time:	2005-175T00:02:35.041	Stop Time:	2005-175T23:59:21.366
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005176_01

Start Time:	2005-176T00:01:21.366	Stop Time:	2005-176T23:57:32.699
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_2005177_01

Start Time:	2005-177T00:00:55.452	Stop Time:	2005-177T23:59:47.390
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005178_01

Start Time:	2005-178T00:02:47.389	Stop Time:	2005-178T23:59:46.839
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005179_01

Start Time:	2005-179T00:02:46.838	Stop Time:	2005-179T23:57:16.711
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005180_01

Start Time:	2005-180T00:00:39.190	Stop Time:	2005-180T23:56:40.496
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005181_01

Start Time:	2005-181T00:00:01.523	Stop Time:	2005-181T23:58:15.820
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005182_01

Start Time:	2005-182T00:01:37.819	Stop Time:	2005-182T23:58:52.035
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_2005183_01

Start Time:	2005-183T00:04:50.033	Stop Time:	2005-183T23:58:35.961
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_2005184_01

Start Time:	2005-184T00:00:35.960	Stop Time:	2005-184T23:59:21.410
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005185_01

Start Time:	2005-185T00:01:21.409	Stop Time:	2005-185T23:58:26.984
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_2005186_01

Start Time:	2005-186T00:01:26.983	Stop Time:	2005-186T23:54:18.834
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005187_01

Start Time:	2005-187T00:00:16.831	Stop Time:	2005-187T23:56:50.641
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005188_01

Start Time:	2005-188T00:00:11.785	Stop Time:	2005-188T23:59:41.332
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_2005189_01

Start Time:	2005-189T00:02:41.331	Stop Time:	2005-189T23:57:42.782
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005190_01

Start Time:	2005-190T00:00:42.781	Stop Time:	2005-190T23:58:58.230
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005191_01

Start Time:	2005-191T00:01:58.229	Stop Time:	2005-191T23:58:34.680
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005192_01

Start Time:	2005-192T00:01:34.679	Stop Time:	2005-192T23:59:15.087
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005193_01

Start Time:	2005-193T00:02:15.085	Stop Time:	2005-193T23:57:11.534
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005194_01

Start Time:	2005-194T00:00:11.533	Stop Time:	2005-194T23:58:22.523
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_2005195_01

Start Time:	2005-195T00:01:44.366	Stop Time:	2005-195T23:58:53.427
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005196_01

Start Time:	2005-196T00:01:53.426	Stop Time:	2005-196T23:59:12.873
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005197_01

Start Time:	2005-197T00:02:12.872	Stop Time:	2005-197T23:59:13.320
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005198_01

Start Time:	2005-198T00:02:13.319	Stop Time:	2005-198T23:58:38.767
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_2005199_01

Start Time:	2005-199T00:01:38.766	Stop Time:	2005-199T23:58:57.213
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005200_01

Start Time:	2005-200T00:01:57.212	Stop Time:	2005-200T18:40:11.782
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005201_01

Start Time:	2005-201T00:25:27.982	Stop Time:	2005-201T23:59:38.106
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005202_01

Start Time:	2005-202T00:02:37.105	Stop Time:	2005-202T23:59:37.553
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005203_01

Start Time:	2005-203T00:02:37.552	Stop Time:	2005-203T23:59:37.000
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005204_01

Start Time:	2005-204T00:02:36.999	Stop Time:	2005-204T23:59:37.447
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005205_01

Start Time:	2005-205T00:02:37.446	Stop Time:	2005-205T23:59:37.894
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005206_01

Start Time:	2005-206T00:02:37.893	Stop Time:	2005-206T23:59:38.341
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005207_01

Start Time:	2005-207T00:02:38.339	Stop Time:	2005-207T23:59:23.787
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_2005208_01

Start Time:	2005-208T00:02:23.786	Stop Time:	2005-208T23:59:38.234
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005209_01

Start Time:	2005-209T00:02:38.233	Stop Time:	2005-209T23:57:57.681
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005210_01

Start Time:	2005-210T00:00:57.680	Stop Time:	2005-210T23:58:45.128
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005211_01

Start Time:	2005-211T00:01:45.126	Stop Time:	2005-211T23:58:45.574
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005212_01

Start Time:	2005-212T00:01:45.573	Stop Time:	2005-212T23:58:46.021
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_2005213_01

Start Time:	2005-213T00:01:46.020	Stop Time:	2005-213T23:58:34.468
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005214_01

Start Time:	2005-214T00:01:34.466	Stop Time:	2005-214T23:57:32.915
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005215_01

Start Time:	2005-215T00:00:32.914	Stop Time:	2005-215T23:57:33.361
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_2005216_01

Start Time:	2005-216T00:00:33.360	Stop Time:	2005-216T23:57:33.808
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005217_01

Start Time:	2005-217T00:00:33.807	Stop Time:	2005-217T23:57:17.255
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_2005218_01

Start Time:	2005-218T00:00:17.254	Stop Time:	2005-218T23:58:16.576
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_2005219_01

Start Time:	2005-219T00:00:16.575	Stop Time:	2005-219T23:59:52.022
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_2005220_01

Start Time:	2005-220T00:01:52.021	Stop Time:	2005-220T23:59:49.469
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005221_01

Start Time:	2005-221T00:01:49.468	Stop Time:	2005-221T23:57:17.041
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005222_01

Start Time:	2005-222T00:00:17.040	Stop Time:	2005-222T23:57:17.488
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005223_01

Start Time:	2005-223T00:00:17.487	Stop Time:	2005-223T23:57:17.935
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005224_01

Start Time:	2005-224T00:00:17.934	Stop Time:	2005-224T23:58:08.381
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_2005225_01

Start Time:	2005-225T00:01:08.380	Stop Time:	2005-225T23:57:21.828
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005226_01

Start Time:	2005-226T00:00:21.827	Stop Time:	2005-226T23:58:47.274
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005227_01

Start Time:	2005-227T00:01:47.273	Stop Time:	2005-227T23:59:14.721
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005228_01

Start Time:	2005-228T00:02:14.719	Stop Time:	2005-228T23:59:17.042
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005229_01

Start Time:	2005-229T00:01:17.041	Stop Time:	2005-229T23:59:53.489
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005230_01

Start Time:	2005-230T00:01:53.488	Stop Time:	2005-230T23:59:19.936
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005231_01

Start Time:	2005-231T00:01:19.935	Stop Time:	2005-231T23:59:18.382
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005232_01

Start Time:	2005-232T00:01:18.381	Stop Time:	2005-232T23:59:47.954
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_2005233_01

Start Time:	2005-233T00:02:47.953	Stop Time:	2005-233T23:58:04.276
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_2005234_01

Start Time:	2005-234T00:00:04.275	Stop Time:	2005-234T23:58:05.723
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005235_01

Start Time:	2005-235T00:00:05.722	Stop Time:	2005-235T23:57:05.295
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005236_01

Start Time:	2005-236T00:00:05.294	Stop Time:	2005-236T23:58:49.741
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_2005237_01

Start Time:	2005-237T00:01:49.740	Stop Time:	2005-237T23:59:00.187
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005238_01

Start Time:	2005-238T00:02:00.186	Stop Time:	2005-238T23:59:00.634
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_2005239_01

Start Time:	2005-239T00:02:00.633	Stop Time:	2005-239T23:57:59.081
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005240_01

Start Time:	2005-240T00:00:59.080	Stop Time:	2005-240T23:58:35.527
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_2005241_01

Start Time:	2005-241T00:01:35.526	Stop Time:	2005-241T23:59:06.849
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005242_01

Start Time:	2005-242T00:01:06.848	Stop Time:	2005-242T23:59:53.295
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005243_01

Start Time:	2005-243T00:01:53.295	Stop Time:	2005-243T23:59:52.867
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005244_01

Start Time:	2005-244T00:02:52.866	Stop Time:	2005-244T17:50:52.455
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_2005245_01

Start Time:	2005-245T03:32:54.232	Stop Time:	2005-245T23:59:05.636
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_2005246_01

Start Time:	2005-246T00:01:05.635	Stop Time:	2005-246T23:59:23.082
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_2005247_01

Start Time:	2005-247T00:01:23.081	Stop Time:	2005-247T23:59:14.529
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005248_01

Start Time:	2005-248T00:01:14.528	Stop Time:	2005-248T23:43:14.982
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_2005249_01

Start Time:	2005-249T10:58:48.843	Stop Time:	2005-249T23:57:26.548
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005250_01

Start Time:	2005-250T00:00:26.547	Stop Time:	2005-250T08:21:25.354
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005251_01

Start Time:	2005-251T02:51:26.928	Stop Time:	2005-251T23:58:18.441
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005252_01

Start Time:	2005-252T00:01:18.440	Stop Time:	2005-252T23:59:35.888
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_2005253_01

Start Time:	2005-253T00:02:35.887	Stop Time:	2005-253T23:59:35.335
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005254_01

Start Time:	2005-254T00:02:35.334	Stop Time:	2005-254T23:59:35.844
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005255_01

Start Time:	2005-255T00:02:35.842	Stop Time:	2005-255T23:59:16.292
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005256_01

Start Time:	2005-256T00:02:16.291	Stop Time:	2005-256T23:59:05.740
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005257_01

Start Time:	2005-257T00:02:05.739	Stop Time:	2005-257T23:58:15.188
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005258_01

Start Time:	2005-258T00:01:15.187	Stop Time:	2005-258T23:58:11.636
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_2005259_01

Start Time:	2005-259T00:01:11.635	Stop Time:	2005-259T23:59:22.084
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_2005260_01

Start Time:	2005-260T00:02:22.082	Stop Time:	2005-260T23:58:45.532
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_2005261_01

Start Time:	2005-261T00:01:45.531	Stop Time:	2005-261T23:58:00.980
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005262_01

Start Time:	2005-262T00:01:00.979	Stop Time:	2005-262T17:28:00.578
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_2005263_01

Start Time:	2005-263T03:10:02.354	Stop Time:	2005-263T23:58:33.751
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005264_01

Start Time:	2005-264T00:00:33.750	Stop Time:	2005-264T23:59:11.199
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_2005265_01

Start Time:	2005-265T00:01:11.198	Stop Time:	2005-265T23:59:51.771
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005266_01

Start Time:	2005-266T00:02:51.770	Stop Time:	2005-266T23:58:21.095
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_2005267_01

Start Time:	2005-267T00:00:21.094	Stop Time:	2005-267T23:57:58.668
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005268_01

Start Time:	2005-268T00:00:58.667	Stop Time:	2005-268T23:57:59.116
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005269_01

Start Time:	2005-269T00:00:59.115	Stop Time:	2005-269T23:57:37.564
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005270_01

Start Time:	2005-270T00:00:37.563	Stop Time:	2005-270T23:59:07.012
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005271_01

Start Time:	2005-271T00:02:07.010	Stop Time:	2005-271T23:59:07.460
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005272_01

Start Time:	2005-272T00:02:07.458	Stop Time:	2005-272T23:57:18.932
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005273_01

Start Time:	2005-273T00:00:40.540	Stop Time:	2005-273T23:57:15.356
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005274_01

Start Time:	2005-274T00:00:15.355	Stop Time:	2005-274T23:57:15.804
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005275_01

Start Time:	2005-275T00:00:15.803	Stop Time:	2005-275T23:57:16.252
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005276_01

Start Time:	2005-276T00:00:16.251	Stop Time:	2005-276T23:57:14.700
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_2005277_01

Start Time:	2005-277T00:00:14.699	Stop Time:	2005-277T23:57:32.148
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005278_01

Start Time:	2005-278T00:00:32.147	Stop Time:	2005-278T23:58:48.596
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005279_01

Start Time:	2005-279T00:01:48.594	Stop Time:	2005-279T23:59:16.918
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005280_01

Start Time:	2005-280T00:01:16.918	Stop Time:	2005-280T23:59:01.366
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005281_01

Start Time:	2005-281T00:01:01.366	Stop Time:	2005-281T23:59:14.439
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005282_01

Start Time:	2005-282T00:00:54.439	Stop Time:	2005-282T23:59:36.262
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_2005283_01

Start Time:	2005-283T00:01:36.261	Stop Time:	2005-283T23:58:29.836
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_2005284_01

Start Time:	2005-284T00:01:29.835	Stop Time:	2005-284T23:58:03.159
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005285_01

Start Time:	2005-285T00:00:03.158	Stop Time:	2005-285T23:57:30.732
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005286_01

Start Time:	2005-286T00:00:30.731	Stop Time:	2005-286T23:59:00.054
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005287_01

Start Time:	2005-287T00:01:00.054	Stop Time:	2005-287T23:58:40.503
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_2005288_01

Start Time:	2005-288T00:00:40.502	Stop Time:	2005-288T23:59:06.950
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_2005289_01

Start Time:	2005-289T00:01:06.950	Stop Time:	2005-289T23:58:19.399
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_2005290_01

Start Time:	2005-290T00:00:19.398	Stop Time:	2005-290T23:58:50.846
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005291_01

Start Time:	2005-291T00:00:50.846	Stop Time:	2005-291T23:59:11.818
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005292_01

Start Time:	2005-292T00:03:18.293	Stop Time:	2005-292T23:59:35.742
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005293_01

Start Time:	2005-293T00:01:35.741	Stop Time:	2005-293T23:59:18.585
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005294_01

Start Time:	2005-294T00:02:39.701	Stop Time:	2005-294T23:58:17.639
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005295_01

Start Time:	2005-295T00:00:16.638	Stop Time:	2005-295T23:58:19.087
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005296_01

Start Time:	2005-296T00:00:19.086	Stop Time:	2005-296T23:58:20.535
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005297_01

Start Time:	2005-297T00:00:20.534	Stop Time:	2005-297T23:58:21.983
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005298_01

Start Time:	2005-298T00:00:21.982	Stop Time:	2005-298T23:58:39.056
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005299_01

Start Time:	2005-299T00:00:19.055	Stop Time:	2005-299T23:59:30.878
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005300_01

Start Time:	2005-300T00:01:30.877	Stop Time:	2005-300T23:59:30.451
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_2005301_01

Start Time:	2005-301T00:02:30.450	Stop Time:	2005-301T23:59:30.899
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_2005302_01

Start Time:	2005-302T00:02:30.898	Stop Time:	2005-302T23:59:20.847
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005303_01

Start Time:	2005-303T00:01:00.847	Stop Time:	2005-303T23:58:40.795
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_2005304_01

Start Time:	2005-304T00:01:40.793	Stop Time:	2005-304T23:59:01.117
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005305_01

Start Time:	2005-305T00:01:01.117	Stop Time:	2005-305T23:59:21.565
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005306_01

Start Time:	2005-306T00:01:21.565	Stop Time:	2005-306T23:59:23.013
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005307_01

Start Time:	2005-307T00:01:23.013	Stop Time:	2005-307T23:57:54.130
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005308_01

Start Time:	2005-308T00:01:15.609	Stop Time:	2005-308T23:59:14.909
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005309_01

Start Time:	2005-309T00:01:14.909	Stop Time:	2005-309T23:57:37.147
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_2005310_01

Start Time:	2005-310T00:00:58.993	Stop Time:	2005-310T23:59:41.930
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005311_01

Start Time:	2005-311T00:02:41.929	Stop Time:	2005-311T23:59:45.253
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005312_01

Start Time:	2005-312T00:01:45.252	Stop Time:	2005-312T23:58:06.702
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_2005313_01

Start Time:	2005-313T00:00:06.701	Stop Time:	2005-313T23:58:39.775
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_2005314_01

Start Time:	2005-314T00:00:19.774	Stop Time:	2005-314T23:58:42.223
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_2005315_01

Start Time:	2005-315T00:00:22.222	Stop Time:	2005-315T23:58:13.046
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005316_01

Start Time:	2005-316T00:00:13.045	Stop Time:	2005-316T23:58:46.119
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005317_01

Start Time:	2005-317T00:00:26.118	Stop Time:	2005-317T23:59:36.941
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005318_01

Start Time:	2005-318T00:01:36.941	Stop Time:	2005-318T23:58:29.015
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_2005319_01

Start Time:	2005-319T00:00:09.014	Stop Time:	2005-319T23:58:31.463
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005320_01

Start Time:	2005-320T00:00:11.462	Stop Time:	2005-320T23:58:10.411
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005321_01

Start Time:	2005-321T00:01:10.410	Stop Time:	2005-321T23:59:46.796
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005322_01

Start Time:	2005-322T00:02:41.369	Stop Time:	2005-322T23:59:58.244
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005323_01

Start Time:	2005-323T00:02:28.243	Stop Time:	2005-323T23:59:06.630
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005324_01

Start Time:	2005-324T00:01:06.629	Stop Time:	2005-324T23:58:57.140
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005325_01

Start Time:	2005-325T00:01:27.139	Stop Time:	2005-325T23:59:19.525
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_2005326_01

Start Time:	2005-326T00:01:19.525	Stop Time:	2005-326T23:58:56.599
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005327_01

Start Time:	2005-327T00:00:36.598	Stop Time:	2005-327T23:58:44.691
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005328_01

Start Time:	2005-328T00:02:06.690	Stop Time:	2005-328T23:58:48.495
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005329_01

Start Time:	2005-329T00:00:28.494	Stop Time:	2005-329T23:57:32.443
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005330_01

Start Time:	2005-330T00:00:32.442	Stop Time:	2005-330T23:57:32.891
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005331_01

Start Time:	2005-331T00:00:32.890	Stop Time:	2005-331T23:57:57.484
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005332_01

Start Time:	2005-332T00:01:18.725	Stop Time:	2005-332T23:58:50.287
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005333_01

Start Time:	2005-333T00:00:30.286	Stop Time:	2005-333T23:59:50.234
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005334_01

Start Time:	2005-334T00:02:50.233	Stop Time:	2005-334T23:59:50.682
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005335_01

Start Time:	2005-335T00:02:50.681	Stop Time:	2005-335T23:58:33.631
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005336_01

Start Time:	2005-336T00:00:13.630	Stop Time:	2005-336T23:59:28.090
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005337_01

Start Time:	2005-337T00:02:48.362	Stop Time:	2005-337T23:59:23.527
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_2005338_01

Start Time:	2005-338T00:01:03.526	Stop Time:	2005-338T23:57:24.475
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005339_01

Start Time:	2005-339T00:00:24.474	Stop Time:	2005-339T23:58:57.923
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_2005340_01

Start Time:	2005-340T00:01:57.922	Stop Time:	2005-340T23:58:08.516
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005341_01

Start Time:	2005-341T00:01:31.639	Stop Time:	2005-341T23:59:53.818
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005342_01

Start Time:	2005-342T00:02:53.817	Stop Time:	2005-342T23:58:39.767
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_2005343_01

Start Time:	2005-343T00:00:19.766	Stop Time:	2005-343T23:57:15.716
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_2005344_01

Start Time:	2005-344T00:00:15.714	Stop Time:	2005-344T23:59:36.100
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_2005345_01

Start Time:	2005-345T00:02:06.099	Stop Time:	2005-345T23:58:55.396
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005346_01

Start Time:	2005-346T00:02:18.367	Stop Time:	2005-346T23:59:03.559
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_2005347_01

Start Time:	2005-347T00:00:43.558	Stop Time:	2005-347T23:58:50.894
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005348_01

Start Time:	2005-348T00:02:12.631	Stop Time:	2005-348T23:58:40.455
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_2005349_01

Start Time:	2005-349T00:00:20.454	Stop Time:	2005-349T23:59:15.611
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005350_01

Start Time:	2005-350T00:02:36.973	Stop Time:	2005-350T23:58:24.288
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005351_01

Start Time:	2005-351T00:00:04.287	Stop Time:	2005-351T23:58:02.745
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005352_01

Start Time:	2005-352T00:01:26.111	Stop Time:	2005-352T23:59:16.179
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005353_01

Start Time:	2005-353T00:00:56.178	Stop Time:	2005-353T23:57:03.395
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005354_01

Start Time:	2005-354T00:00:23.191	Stop Time:	2005-354T23:59:26.445
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005355_01

Start Time:	2005-355T00:01:26.445	Stop Time:	2005-355T23:59:27.891
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005356_01

Start Time:	2005-356T00:01:27.891	Stop Time:	2005-356T23:56:46.975
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005357_01

Start Time:	2005-357T00:00:09.220	Stop Time:	2005-357T23:58:47.409
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005358_01

Start Time:	2005-358T00:00:27.408	Stop Time:	2005-358T23:58:50.855
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_2005359_01

Start Time:	2005-359T00:00:30.854	Stop Time:	2005-359T23:57:02.071
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_2005360_01

Start Time:	2005-360T00:00:21.343	Stop Time:	2005-360T23:58:47.747
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005361_01

Start Time:	2005-361T00:00:27.746	Stop Time:	2005-361T23:58:01.568
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005362_01

Start Time:	2005-362T00:00:01.567	Stop Time:	2005-362T23:59:07.014
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_2005363_01

Start Time:	2005-363T00:01:07.013	Stop Time:	2005-363T23:58:14.523
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_2005364_01

Start Time:	2005-364T00:00:44.522	Stop Time:	2005-364T23:59:29.031
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2005365_01

Start Time:	2005-365T00:02:29.030	Stop Time:	2005-365T23:59:29.477
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.

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