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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/ 2016 /

CMFULL0_2016001_01

Start Time:	2016-001T00:00:15.832	Stop Time:	2016-001T23:58:08.282
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016002_01

Start Time:	2016-002T00:00:08.281	Stop Time:	2016-002T23:57:15.434
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016003_01

Start Time:	2016-003T00:01:33.187	Stop Time:	2016-003T23:57:34.305
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016004_01

Start Time:	2016-004T00:00:34.304	Stop Time:	2016-004T23:59:09.754
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016005_01

Start Time:	2016-005T00:02:09.753	Stop Time:	2016-005T23:59:10.203
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016006_01

Start Time:	2016-006T00:02:10.202	Stop Time:	2016-006T23:58:42.652
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016007_01

Start Time:	2016-007T00:01:42.651	Stop Time:	2016-007T23:58:42.101
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016008_01

Start Time:	2016-008T00:01:42.100	Stop Time:	2016-008T23:58:20.551
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016009_01

Start Time:	2016-009T00:01:20.549	Stop Time:	2016-009T23:59:48.741
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_2016010_01

Start Time:	2016-010T00:04:04.330	Stop Time:	2016-010T23:58:17.414
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016011_01

Start Time:	2016-011T00:02:32.799	Stop Time:	2016-011T23:55:57.641
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_2016012_01

Start Time:	2016-012T00:00:12.862	Stop Time:	2016-012T23:59:17.347
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_2016013_01

Start Time:	2016-013T00:02:17.346	Stop Time:	2016-013T23:59:19.671
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016014_01

Start Time:	2016-014T00:01:19.670	Stop Time:	2016-014T23:58:48.245
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_2016015_01

Start Time:	2016-015T00:01:48.244	Stop Time:	2016-015T23:59:57.694
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016016_01

Start Time:	2016-016T00:02:57.693	Stop Time:	2016-016T23:58:41.108
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_2016017_01

Start Time:	2016-017T00:02:57.079	Stop Time:	2016-017T23:57:25.593
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016018_01

Start Time:	2016-018T00:00:25.592	Stop Time:	2016-018T23:58:26.042
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_2016019_01

Start Time:	2016-019T00:01:26.041	Stop Time:	2016-019T23:58:26.491
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016020_01

Start Time:	2016-020T00:01:26.490	Stop Time:	2016-020T23:56:17.293
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016021_01

Start Time:	2016-021T00:00:32.709	Stop Time:	2016-021T21:23:15.448
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_2016022_01

Start Time:	2016-022T01:38:49.350	Stop Time:	2016-022T23:58:19.381
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_2016023_01

Start Time:	2016-023T00:02:36.383	Stop Time:	2016-023T23:59:41.286
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016024_01

Start Time:	2016-024T00:02:41.285	Stop Time:	2016-024T23:59:13.736
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016025_01

Start Time:	2016-025T00:02:13.734	Stop Time:	2016-025T01:29:13.701
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016026_01

Start Time:	2016-026T01:14:00.156	Stop Time:	2016-026T23:55:57.791
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016027_01

Start Time:	2016-027T00:00:12.790	Stop Time:	2016-027T23:57:55.240
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_2016028_01

Start Time:	2016-028T00:02:12.215	Stop Time:	2016-028T23:59:33.532
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_2016029_01

Start Time:	2016-029T00:02:33.531	Stop Time:	2016-029T23:59:38.856
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016030_01

Start Time:	2016-030T00:01:38.855	Stop Time:	2016-030T23:58:38.431
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016031_01

Start Time:	2016-031T00:01:38.429	Stop Time:	2016-031T23:58:54.817
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016032_01

Start Time:	2016-032T00:00:56.691	Stop Time:	2016-032T23:59:39.328
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016033_01

Start Time:	2016-033T00:02:39.327	Stop Time:	2016-033T23:59:21.778
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016034_01

Start Time:	2016-034T00:02:21.777	Stop Time:	2016-034T23:57:01.228
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016035_01

Start Time:	2016-035T00:00:01.227	Stop Time:	2016-035T19:29:11.717
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016036_01

Start Time:	2016-036T00:20:53.668	Stop Time:	2016-036T23:58:13.657
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016037_01

Start Time:	2016-037T00:02:31.257	Stop Time:	2016-037T23:57:00.575
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016038_01

Start Time:	2016-038T00:00:00.574	Stop Time:	2016-038T23:59:56.614
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016039_01

Start Time:	2016-039T00:03:37.683	Stop Time:	2016-039T23:57:37.121
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_2016040_01

Start Time:	2016-040T00:00:37.120	Stop Time:	2016-040T23:57:37.558
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016041_01

Start Time:	2016-041T00:00:37.557	Stop Time:	2016-041T23:57:37.994
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016042_01

Start Time:	2016-042T00:00:37.993	Stop Time:	2016-042T23:57:37.430
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016043_01

Start Time:	2016-043T00:00:37.429	Stop Time:	2016-043T23:57:37.867
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_2016044_01

Start Time:	2016-044T00:00:37.866	Stop Time:	2016-044T23:57:37.303
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016045_01

Start Time:	2016-045T00:00:37.302	Stop Time:	2016-045T23:58:09.614
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016046_01

Start Time:	2016-046T00:00:09.613	Stop Time:	2016-046T23:59:41.050
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016047_01

Start Time:	2016-047T00:01:41.049	Stop Time:	2016-047T23:59:42.424
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016048_01

Start Time:	2016-048T00:01:12.423	Stop Time:	2016-048T23:57:55.052
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016049_01

Start Time:	2016-049T00:02:10.593	Stop Time:	2016-049T23:59:46.640
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016050_01

Start Time:	2016-050T00:04:01.638	Stop Time:	2016-050T23:57:54.921
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016051_01

Start Time:	2016-051T00:00:54.920	Stop Time:	2016-051T23:57:42.357
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016052_01

Start Time:	2016-052T00:00:42.356	Stop Time:	2016-052T23:57:42.794
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016053_01

Start Time:	2016-053T00:00:42.792	Stop Time:	2016-053T23:59:52.229
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016054_01

Start Time:	2016-054T00:02:52.228	Stop Time:	2016-054T23:59:52.665
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016055_01

Start Time:	2016-055T00:02:52.664	Stop Time:	2016-055T23:58:33.102
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_2016056_01

Start Time:	2016-056T00:01:33.101	Stop Time:	2016-056T23:58:32.539
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016057_01

Start Time:	2016-057T00:01:32.537	Stop Time:	2016-057T23:59:00.975
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_2016058_01

Start Time:	2016-058T00:02:00.974	Stop Time:	2016-058T23:58:05.411
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_2016059_01

Start Time:	2016-059T00:01:05.410	Stop Time:	2016-059T23:59:03.847
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_2016060_01

Start Time:	2016-060T00:02:03.846	Stop Time:	2016-060T23:59:04.284
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016061_01

Start Time:	2016-061T00:02:04.282	Stop Time:	2016-061T23:59:03.720
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016062_01

Start Time:	2016-062T00:02:03.719	Stop Time:	2016-062T23:59:04.156
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016063_01

Start Time:	2016-063T00:02:04.155	Stop Time:	2016-063T23:59:03.593
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016064_01

Start Time:	2016-064T00:02:03.591	Stop Time:	2016-064T23:59:04.029
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_2016065_01

Start Time:	2016-065T00:02:04.028	Stop Time:	2016-065T23:59:13.465
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016066_01

Start Time:	2016-066T00:02:13.464	Stop Time:	2016-066T09:56:13.231
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016068_01

Start Time:	2016-068T12:02:15.055	Stop Time:	2016-068T23:59:13.774
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016069_01

Start Time:	2016-069T00:02:13.773	Stop Time:	2016-069T23:58:16.085
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016070_01

Start Time:	2016-070T00:00:16.084	Stop Time:	2016-070T23:58:04.521
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016071_01

Start Time:	2016-071T00:00:04.520	Stop Time:	2016-071T23:59:35.144
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_2016072_01

Start Time:	2016-072T00:03:05.143	Stop Time:	2016-072T23:58:07.581
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016073_01

Start Time:	2016-073T00:01:37.580	Stop Time:	2016-073T23:57:07.112
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016074_01

Start Time:	2016-074T00:01:22.110	Stop Time:	2016-074T23:57:52.548
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_2016075_01

Start Time:	2016-075T00:02:07.546	Stop Time:	2016-075T23:59:46.983
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_2016076_01

Start Time:	2016-076T00:04:01.982	Stop Time:	2016-076T23:56:16.421
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016077_01

Start Time:	2016-077T00:00:31.419	Stop Time:	2016-077T23:57:44.857
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016078_01

Start Time:	2016-078T00:01:59.855	Stop Time:	2016-078T23:58:30.293
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016079_01

Start Time:	2016-079T00:02:45.291	Stop Time:	2016-079T23:59:10.573
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016080_01

Start Time:	2016-080T00:02:10.571	Stop Time:	2016-080T23:59:11.009
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_2016081_01

Start Time:	2016-081T00:02:11.008	Stop Time:	2016-081T23:56:28.603
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016082_01

Start Time:	2016-082T00:00:43.601	Stop Time:	2016-082T23:57:14.039
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016083_01

Start Time:	2016-083T00:01:29.037	Stop Time:	2016-083T23:58:54.474
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016084_01

Start Time:	2016-084T00:03:09.473	Stop Time:	2016-084T23:56:37.911
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016085_01

Start Time:	2016-085T00:00:52.910	Stop Time:	2016-085T23:58:01.347
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_2016086_01

Start Time:	2016-086T00:02:16.346	Stop Time:	2016-086T23:59:33.627
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016087_01

Start Time:	2016-087T00:02:33.625	Stop Time:	2016-087T23:59:34.063
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016088_01

Start Time:	2016-088T00:02:34.062	Stop Time:	2016-088T23:59:14.499
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016089_01

Start Time:	2016-089T00:02:14.498	Stop Time:	2016-089T23:58:52.936
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_2016090_01

Start Time:	2016-090T00:01:52.935	Stop Time:	2016-090T23:58:37.528
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016091_01

Start Time:	2016-091T00:02:52.527	Stop Time:	2016-091T23:57:24.809
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016092_01

Start Time:	2016-092T00:00:24.808	Stop Time:	2016-092T23:57:25.245
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_2016093_01

Start Time:	2016-093T00:00:25.244	Stop Time:	2016-093T23:57:25.682
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_2016094_01

Start Time:	2016-094T00:00:25.680	Stop Time:	2016-094T23:57:26.118
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016095_01

Start Time:	2016-095T00:00:26.117	Stop Time:	2016-095T23:57:56.554
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016096_01

Start Time:	2016-096T00:00:56.553	Stop Time:	2016-096T23:57:55.990
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016097_01

Start Time:	2016-097T00:00:55.989	Stop Time:	2016-097T23:58:26.426
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016098_01

Start Time:	2016-098T00:01:26.425	Stop Time:	2016-098T23:59:26.862
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016099_01

Start Time:	2016-099T00:02:26.861	Stop Time:	2016-099T23:59:27.299
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016100_01

Start Time:	2016-100T00:02:27.297	Stop Time:	2016-100T23:59:27.735
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016101_01

Start Time:	2016-101T00:02:27.734	Stop Time:	2016-101T23:59:39.171
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016102_01

Start Time:	2016-102T00:02:39.170	Stop Time:	2016-102T23:59:39.607
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016103_01

Start Time:	2016-103T00:02:39.606	Stop Time:	2016-103T23:59:44.044
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016104_01

Start Time:	2016-104T00:02:44.043	Stop Time:	2016-104T23:59:44.480
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_2016105_01

Start Time:	2016-105T00:02:44.479	Stop Time:	2016-105T23:57:04.917
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016106_01

Start Time:	2016-106T00:00:04.916	Stop Time:	2016-106T23:57:04.354
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_2016107_01

Start Time:	2016-107T00:00:04.353	Stop Time:	2016-107T23:57:42.790
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_2016108_01

Start Time:	2016-108T00:00:42.789	Stop Time:	2016-108T23:57:42.226
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016109_01

Start Time:	2016-109T00:00:42.225	Stop Time:	2016-109T23:56:01.979
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_2016110_01

Start Time:	2016-110T00:00:17.782	Stop Time:	2016-110T23:58:17.073
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016111_01

Start Time:	2016-111T00:01:17.072	Stop Time:	2016-111T23:57:59.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016112_01

Start Time:	2016-112T00:00:59.519	Stop Time:	2016-112T23:57:08.967
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016113_01

Start Time:	2016-113T00:00:08.965	Stop Time:	2016-113T23:56:08.183
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016114_01

Start Time:	2016-114T00:00:23.568	Stop Time:	2016-114T23:57:09.860
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016115_01

Start Time:	2016-115T00:00:09.858	Stop Time:	2016-115T23:57:10.306
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016116_01

Start Time:	2016-116T00:00:10.305	Stop Time:	2016-116T23:57:10.752
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016117_01

Start Time:	2016-117T00:00:10.751	Stop Time:	2016-117T23:57:10.199
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_2016118_01

Start Time:	2016-118T00:00:10.198	Stop Time:	2016-118T23:57:10.645
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016119_01

Start Time:	2016-119T00:00:10.644	Stop Time:	2016-119T23:57:10.092
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_2016120_01

Start Time:	2016-120T00:00:10.091	Stop Time:	2016-120T23:57:10.539
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016121_01

Start Time:	2016-121T00:00:10.538	Stop Time:	2016-121T23:57:10.986
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016122_01

Start Time:	2016-122T00:00:10.984	Stop Time:	2016-122T23:57:10.432
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016123_01

Start Time:	2016-123T00:00:11.431	Stop Time:	2016-123T23:57:10.878
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_2016124_01

Start Time:	2016-124T00:00:10.877	Stop Time:	2016-124T23:57:11.325
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016125_01

Start Time:	2016-125T00:00:11.324	Stop Time:	2016-125T23:58:38.646
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016126_01

Start Time:	2016-126T00:00:38.645	Stop Time:	2016-126T23:59:29.217
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016127_01

Start Time:	2016-127T00:02:29.216	Stop Time:	2016-127T23:59:29.663
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016128_01

Start Time:	2016-128T00:02:29.662	Stop Time:	2016-128T23:58:50.110
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016129_01

Start Time:	2016-129T00:01:50.109	Stop Time:	2016-129T23:58:36.557
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016130_01

Start Time:	2016-130T00:01:36.555	Stop Time:	2016-130T23:58:37.003
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016131_01

Start Time:	2016-131T00:01:37.002	Stop Time:	2016-131T23:58:13.450
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016132_01

Start Time:	2016-132T00:01:13.448	Stop Time:	2016-132T23:58:12.896
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016133_01

Start Time:	2016-133T00:01:12.895	Stop Time:	2016-133T23:58:24.342
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016134_01

Start Time:	2016-134T00:25:24.332	Stop Time:	2016-134T23:58:23.789
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016135_01

Start Time:	2016-135T00:25:23.778	Stop Time:	2016-135T23:58:24.235
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016136_01

Start Time:	2016-136T00:25:24.225	Stop Time:	2016-136T23:58:23.682
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_2016137_01

Start Time:	2016-137T00:25:23.671	Stop Time:	2016-137T23:56:08.898
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016138_01

Start Time:	2016-138T00:00:23.092	Stop Time:	2016-138T23:56:11.732
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_2016139_01

Start Time:	2016-139T00:00:25.960	Stop Time:	2016-139T23:57:25.021
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_2016140_01

Start Time:	2016-140T00:00:25.020	Stop Time:	2016-140T23:57:25.468
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_2016141_01

Start Time:	2016-141T00:00:25.467	Stop Time:	2016-141T23:57:25.914
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016142_01

Start Time:	2016-142T00:00:25.913	Stop Time:	2016-142T23:57:25.361
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_2016143_01

Start Time:	2016-143T00:00:25.359	Stop Time:	2016-143T23:57:25.807
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016144_01

Start Time:	2016-144T00:00:25.806	Stop Time:	2016-144T01:54:24.762
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016150_01

Start Time:	2016-150T22:34:49.433	Stop Time:	2016-150T23:56:28.401
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016151_01

Start Time:	2016-151T00:00:35.462	Stop Time:	2016-151T23:57:22.343
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016152_01

Start Time:	2016-152T00:01:36.764	Stop Time:	2016-152T23:56:34.372
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016153_01

Start Time:	2016-153T00:00:50.370	Stop Time:	2016-153T23:59:11.271
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016154_01

Start Time:	2016-154T00:02:11.269	Stop Time:	2016-154T23:57:38.718
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016155_01

Start Time:	2016-155T00:00:38.716	Stop Time:	2016-155T23:59:50.163
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016156_01

Start Time:	2016-156T00:02:50.162	Stop Time:	2016-156T23:59:24.610
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016157_01

Start Time:	2016-157T00:02:24.609	Stop Time:	2016-157T23:58:56.931
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016158_01

Start Time:	2016-158T00:00:56.931	Stop Time:	2016-158T23:59:21.635
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_2016159_01

Start Time:	2016-159T00:03:38.243	Stop Time:	2016-159T23:57:58.887
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016160_01

Start Time:	2016-160T00:00:28.886	Stop Time:	2016-160T23:58:59.333
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016161_01

Start Time:	2016-161T00:01:29.332	Stop Time:	2016-161T23:59:33.842
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016162_01

Start Time:	2016-162T00:02:33.841	Stop Time:	2016-162T23:59:51.288
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_2016163_01

Start Time:	2016-163T00:02:51.287	Stop Time:	2016-163T23:59:30.735
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016164_01

Start Time:	2016-164T00:02:30.734	Stop Time:	2016-164T23:59:13.181
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016165_01

Start Time:	2016-165T00:02:13.180	Stop Time:	2016-165T23:59:13.628
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016166_01

Start Time:	2016-166T00:02:13.627	Stop Time:	2016-166T23:59:32.074
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016167_01

Start Time:	2016-167T00:02:32.073	Stop Time:	2016-167T23:59:32.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016168_01

Start Time:	2016-168T00:02:32.519	Stop Time:	2016-168T23:59:21.968
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016169_01

Start Time:	2016-169T00:02:21.967	Stop Time:	2016-169T23:59:22.414
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016170_01

Start Time:	2016-170T00:02:22.413	Stop Time:	2016-170T23:59:22.861
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016171_01

Start Time:	2016-171T00:02:22.860	Stop Time:	2016-171T23:59:22.307
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016172_01

Start Time:	2016-172T00:02:22.306	Stop Time:	2016-172T23:59:22.754
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016173_01

Start Time:	2016-173T00:02:22.752	Stop Time:	2016-173T23:59:22.200
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016174_01

Start Time:	2016-174T00:02:22.199	Stop Time:	2016-174T23:59:22.646
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016175_01

Start Time:	2016-175T00:02:22.645	Stop Time:	2016-175T23:59:23.093
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016176_01

Start Time:	2016-176T00:02:23.092	Stop Time:	2016-176T23:59:22.539
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016177_01

Start Time:	2016-177T00:02:22.538	Stop Time:	2016-177T23:59:22.986
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016178_01

Start Time:	2016-178T00:02:22.985	Stop Time:	2016-178T23:59:23.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016179_01

Start Time:	2016-179T00:02:23.519	Stop Time:	2016-179T23:58:41.969
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016180_01

Start Time:	2016-180T00:01:41.968	Stop Time:	2016-180T23:58:39.417
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016181_01

Start Time:	2016-181T00:01:39.416	Stop Time:	2016-181T23:57:12.413
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016182_01

Start Time:	2016-182T00:01:29.395	Stop Time:	2016-182T23:56:46.084
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_2016183_01

Start Time:	2016-183T00:01:00.664	Stop Time:	2016-183T23:58:33.637
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016184_01

Start Time:	2016-184T00:00:33.636	Stop Time:	2016-184T23:59:40.209
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016185_01

Start Time:	2016-185T00:02:40.208	Stop Time:	2016-185T23:59:40.658
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016186_01

Start Time:	2016-186T00:02:40.656	Stop Time:	2016-186T23:59:40.106
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_2016187_01

Start Time:	2016-187T00:02:40.105	Stop Time:	2016-187T23:58:16.555
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016188_01

Start Time:	2016-188T00:01:16.553	Stop Time:	2016-188T23:59:45.002
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016189_01

Start Time:	2016-189T00:02:45.001	Stop Time:	2016-189T23:59:39.451
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_2016190_01

Start Time:	2016-190T00:02:39.449	Stop Time:	2016-190T23:58:05.899
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_2016191_01

Start Time:	2016-191T00:01:05.898	Stop Time:	2016-191T23:58:06.348
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016192_01

Start Time:	2016-192T00:01:06.346	Stop Time:	2016-192T23:58:05.796
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_2016193_01

Start Time:	2016-193T00:01:05.795	Stop Time:	2016-193T23:58:06.244
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_2016194_01

Start Time:	2016-194T00:01:06.243	Stop Time:	2016-194T23:58:06.692
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016195_01

Start Time:	2016-195T00:01:06.691	Stop Time:	2016-195T23:58:06.140
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_2016196_01

Start Time:	2016-196T00:01:06.139	Stop Time:	2016-196T23:58:06.589
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016197_01

Start Time:	2016-197T00:01:06.588	Stop Time:	2016-197T23:58:07.037
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016198_01

Start Time:	2016-198T00:01:07.036	Stop Time:	2016-198T23:58:06.485
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016199_01

Start Time:	2016-199T00:01:06.484	Stop Time:	2016-199T23:57:38.934
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_2016200_01

Start Time:	2016-200T00:00:38.932	Stop Time:	2016-200T23:57:02.382
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_2016201_01

Start Time:	2016-201T00:00:02.381	Stop Time:	2016-201T23:58:34.377
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_2016202_01

Start Time:	2016-202T00:02:51.570	Stop Time:	2016-202T23:57:02.278
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016203_01

Start Time:	2016-203T00:00:02.277	Stop Time:	2016-203T23:59:19.726
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016204_01

Start Time:	2016-204T00:02:19.725	Stop Time:	2016-204T23:58:53.175
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016205_01

Start Time:	2016-205T00:01:53.174	Stop Time:	2016-205T23:56:06.781
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016206_01

Start Time:	2016-206T00:00:21.779	Stop Time:	2016-206T23:57:25.072
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_2016207_01

Start Time:	2016-207T00:00:25.071	Stop Time:	2016-207T23:57:25.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016208_01

Start Time:	2016-208T00:00:25.519	Stop Time:	2016-208T23:57:10.969
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016209_01

Start Time:	2016-209T00:00:10.968	Stop Time:	2016-209T23:59:10.416
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016210_01

Start Time:	2016-210T00:02:10.415	Stop Time:	2016-210T23:57:13.865
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016211_01

Start Time:	2016-211T00:00:13.864	Stop Time:	2016-211T23:59:56.312
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_2016212_01

Start Time:	2016-212T00:02:56.311	Stop Time:	2016-212T23:55:46.895
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016213_01

Start Time:	2016-213T00:00:04.292	Stop Time:	2016-213T23:57:13.210
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016214_01

Start Time:	2016-214T00:00:13.209	Stop Time:	2016-214T23:59:45.657
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016215_01

Start Time:	2016-215T00:02:45.656	Stop Time:	2016-215T23:59:19.105
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016216_01

Start Time:	2016-216T00:02:19.104	Stop Time:	2016-216T23:58:50.554
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016217_01

Start Time:	2016-217T00:01:50.553	Stop Time:	2016-217T23:59:13.002
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016218_01

Start Time:	2016-218T00:02:13.001	Stop Time:	2016-218T23:57:51.451
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_2016219_01

Start Time:	2016-219T00:00:51.450	Stop Time:	2016-219T23:57:34.899
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_2016220_01

Start Time:	2016-220T00:00:34.898	Stop Time:	2016-220T23:58:44.222
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016221_01

Start Time:	2016-221T00:00:44.221	Stop Time:	2016-221T23:58:50.795
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_2016222_01

Start Time:	2016-222T00:01:50.794	Stop Time:	2016-222T23:59:04.243
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016223_01

Start Time:	2016-223T00:02:04.242	Stop Time:	2016-223T23:59:49.691
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_2016224_01

Start Time:	2016-224T00:02:49.690	Stop Time:	2016-224T23:58:50.140
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_2016225_01

Start Time:	2016-225T00:01:50.139	Stop Time:	2016-225T23:58:49.588
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016226_01

Start Time:	2016-226T00:01:49.587	Stop Time:	2016-226T23:59:15.036
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016227_01

Start Time:	2016-227T00:02:15.035	Stop Time:	2016-227T23:58:50.484
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_2016228_01

Start Time:	2016-228T00:01:50.483	Stop Time:	2016-228T23:58:21.933
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_2016229_01

Start Time:	2016-229T00:01:21.932	Stop Time:	2016-229T23:58:01.381
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_2016230_01

Start Time:	2016-230T00:01:01.380	Stop Time:	2016-230T23:59:58.829
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016231_01

Start Time:	2016-231T00:02:58.828	Stop Time:	2016-231T23:57:42.278
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016232_01

Start Time:	2016-232T00:00:42.277	Stop Time:	2016-232T23:59:44.600
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016233_01

Start Time:	2016-233T00:01:44.599	Stop Time:	2016-233T23:58:30.049
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016234_01

Start Time:	2016-234T00:00:30.048	Stop Time:	2016-234T23:58:28.622
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016235_01

Start Time:	2016-235T00:01:28.621	Stop Time:	2016-235T23:58:28.070
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016236_01

Start Time:	2016-236T00:01:28.069	Stop Time:	2016-236T23:57:07.519
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016237_01

Start Time:	2016-237T00:00:07.518	Stop Time:	2016-237T23:57:07.967
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016238_01

Start Time:	2016-238T00:00:07.966	Stop Time:	2016-238T23:57:04.416
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016239_01

Start Time:	2016-239T00:00:04.414	Stop Time:	2016-239T23:57:03.864
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016240_01

Start Time:	2016-240T00:00:03.863	Stop Time:	2016-240T23:58:46.311
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016241_01

Start Time:	2016-241T00:01:46.310	Stop Time:	2016-241T23:58:46.760
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_2016242_01

Start Time:	2016-242T00:01:46.759	Stop Time:	2016-242T23:58:20.208
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016243_01

Start Time:	2016-243T00:01:20.207	Stop Time:	2016-243T23:58:20.656
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016244_01

Start Time:	2016-244T00:01:20.655	Stop Time:	2016-244T23:59:52.979
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_2016245_01

Start Time:	2016-245T00:01:52.978	Stop Time:	2016-245T23:59:20.427
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_2016246_01

Start Time:	2016-246T00:01:20.427	Stop Time:	2016-246T23:59:59.875
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016247_01

Start Time:	2016-247T00:01:59.875	Stop Time:	2016-247T23:58:28.449
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_2016248_01

Start Time:	2016-248T00:01:28.448	Stop Time:	2016-248T23:58:21.054
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_2016249_01

Start Time:	2016-249T00:02:36.052	Stop Time:	2016-249T09:44:49.829
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016250_01

Start Time:	2016-250T01:45:21.461	Stop Time:	2016-250T23:59:50.950
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_2016251_01

Start Time:	2016-251T00:04:05.948	Stop Time:	2016-251T23:56:21.399
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_2016252_01

Start Time:	2016-252T00:00:36.398	Stop Time:	2016-252T23:57:06.716
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_2016253_01

Start Time:	2016-253T00:01:21.715	Stop Time:	2016-253T23:57:52.164
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016254_01

Start Time:	2016-254T00:02:07.162	Stop Time:	2016-254T23:58:39.454
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016255_01

Start Time:	2016-255T00:01:39.453	Stop Time:	2016-255T23:59:35.900
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016256_01

Start Time:	2016-256T00:02:35.899	Stop Time:	2016-256T23:59:36.347
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_2016257_01

Start Time:	2016-257T00:02:36.346	Stop Time:	2016-257T23:59:36.794
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016258_01

Start Time:	2016-258T00:02:36.793	Stop Time:	2016-258T23:59:07.116
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_2016259_01

Start Time:	2016-259T00:01:07.115	Stop Time:	2016-259T23:58:05.688
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016260_01

Start Time:	2016-260T00:01:05.687	Stop Time:	2016-260T23:58:20.135
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016261_01

Start Time:	2016-261T00:01:20.134	Stop Time:	2016-261T23:57:04.582
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016262_01

Start Time:	2016-262T00:00:04.581	Stop Time:	2016-262T23:58:49.029
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_2016263_01

Start Time:	2016-263T00:01:49.027	Stop Time:	2016-263T23:58:19.476
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016264_01

Start Time:	2016-264T00:01:19.475	Stop Time:	2016-264T23:58:18.923
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016265_01

Start Time:	2016-265T00:01:18.921	Stop Time:	2016-265T23:58:39.369
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_2016266_01

Start Time:	2016-266T00:01:39.368	Stop Time:	2016-266T23:57:21.973
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016267_01

Start Time:	2016-267T00:01:36.971	Stop Time:	2016-267T23:58:07.419
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016268_01

Start Time:	2016-268T00:02:22.418	Stop Time:	2016-268T23:59:53.772
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016269_01

Start Time:	2016-269T00:03:23.770	Stop Time:	2016-269T23:58:16.313
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016270_01

Start Time:	2016-270T00:02:31.311	Stop Time:	2016-270T23:59:01.603
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016271_01

Start Time:	2016-271T00:02:01.602	Stop Time:	2016-271T23:59:02.050
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016272_01

Start Time:	2016-272T00:02:02.049	Stop Time:	2016-272T23:59:01.497
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016273_01

Start Time:	2016-273T00:02:01.496	Stop Time:	2016-273T23:59:02.944
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016274_01

Start Time:	2016-274T00:02:01.943	Stop Time:	2016-274T23:58:47.391
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016275_01

Start Time:	2016-275T00:01:47.390	Stop Time:	2016-275T23:58:19.838
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016276_01

Start Time:	2016-276T00:01:19.837	Stop Time:	2016-276T23:57:12.285
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016277_01

Start Time:	2016-277T00:00:12.284	Stop Time:	2016-277T23:57:12.732
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_2016278_01

Start Time:	2016-278T00:00:12.731	Stop Time:	2016-278T23:58:53.178
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016279_01

Start Time:	2016-279T00:01:53.177	Stop Time:	2016-279T23:58:49.625
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016280_01

Start Time:	2016-280T00:01:49.624	Stop Time:	2016-280T23:58:35.947
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_2016281_01

Start Time:	2016-281T00:00:35.946	Stop Time:	2016-281T23:58:35.519
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016282_01

Start Time:	2016-282T00:01:35.518	Stop Time:	2016-282T23:59:51.965
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016283_01

Start Time:	2016-283T00:02:51.964	Stop Time:	2016-283T23:59:50.350
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016284_01

Start Time:	2016-284T00:04:07.942	Stop Time:	2016-284T23:58:35.859
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016285_01

Start Time:	2016-285T00:01:35.858	Stop Time:	2016-285T23:59:56.306
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016286_01

Start Time:	2016-286T00:02:56.305	Stop Time:	2016-286T23:59:08.815
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_2016287_01

Start Time:	2016-287T00:02:38.814	Stop Time:	2016-287T23:59:26.262
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_2016288_01

Start Time:	2016-288T00:02:56.261	Stop Time:	2016-288T23:59:10.709
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016289_01

Start Time:	2016-289T00:02:40.708	Stop Time:	2016-289T23:57:01.446
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016290_01

Start Time:	2016-290T00:01:18.030	Stop Time:	2016-290T23:56:00.698
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016291_01

Start Time:	2016-291T00:00:15.696	Stop Time:	2016-291T23:59:01.143
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016292_01

Start Time:	2016-292T00:03:16.142	Stop Time:	2016-292T23:59:45.590
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016293_01

Start Time:	2016-293T00:03:59.588	Stop Time:	2016-293T23:56:16.038
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016294_01

Start Time:	2016-294T00:00:31.037	Stop Time:	2016-294T23:57:01.485
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016295_01

Start Time:	2016-295T00:01:16.483	Stop Time:	2016-295T23:57:45.931
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016296_01

Start Time:	2016-296T00:02:00.930	Stop Time:	2016-296T23:57:54.378
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016297_01

Start Time:	2016-297T00:02:09.376	Stop Time:	2016-297T23:58:31.606
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016298_01

Start Time:	2016-298T00:02:45.245	Stop Time:	2016-298T23:56:54.858
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016299_01

Start Time:	2016-299T00:01:12.052	Stop Time:	2016-299T23:59:47.562
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016300_01

Start Time:	2016-300T00:02:47.561	Stop Time:	2016-300T23:56:40.014
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_2016301_01

Start Time:	2016-301T00:00:20.008	Stop Time:	2016-301T23:59:17.612
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016302_01

Start Time:	2016-302T00:03:32.610	Stop Time:	2016-302T23:59:15.235
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016303_01

Start Time:	2016-303T00:03:32.034	Stop Time:	2016-303T23:55:48.507
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016304_01

Start Time:	2016-304T00:00:03.505	Stop Time:	2016-304T23:57:30.796
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_2016305_01

Start Time:	2016-305T00:00:30.795	Stop Time:	2016-305T23:58:42.242
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016306_01

Start Time:	2016-306T00:01:42.241	Stop Time:	2016-306T23:57:55.654
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016307_01

Start Time:	2016-307T00:02:10.075	Stop Time:	2016-307T23:59:46.136
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016308_01

Start Time:	2016-308T00:02:46.134	Stop Time:	2016-308T23:56:35.521
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016309_01

Start Time:	2016-309T00:00:53.934	Stop Time:	2016-309T23:58:28.905
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_2016310_01

Start Time:	2016-310T00:00:28.904	Stop Time:	2016-310T23:57:14.055
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016311_01

Start Time:	2016-311T00:01:27.054	Stop Time:	2016-311T23:57:02.924
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016312_01

Start Time:	2016-312T00:00:02.923	Stop Time:	2016-312T23:58:22.370
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016313_01

Start Time:	2016-313T00:01:22.369	Stop Time:	2016-313T23:59:58.817
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016314_01

Start Time:	2016-314T00:02:58.816	Stop Time:	2016-314T23:58:39.420
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016315_01

Start Time:	2016-315T00:02:54.227	Stop Time:	2016-315T23:56:33.063
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016316_01

Start Time:	2016-316T00:00:48.480	Stop Time:	2016-316T23:58:35.033
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016317_01

Start Time:	2016-317T00:00:35.032	Stop Time:	2016-317T23:58:34.374
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016318_01

Start Time:	2016-318T00:02:49.150	Stop Time:	2016-318T23:59:14.864
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016319_01

Start Time:	2016-319T00:00:44.863	Stop Time:	2016-319T23:57:01.437
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016320_01

Start Time:	2016-320T00:01:16.849	Stop Time:	2016-320T23:55:55.493
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016321_01

Start Time:	2016-321T00:00:11.077	Stop Time:	2016-321T23:56:38.744
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016322_01

Start Time:	2016-322T00:00:53.778	Stop Time:	2016-322T23:59:42.839
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_2016323_01

Start Time:	2016-323T00:02:42.837	Stop Time:	2016-323T23:59:42.285
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016324_01

Start Time:	2016-324T00:02:42.284	Stop Time:	2016-324T23:59:45.607
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016325_01

Start Time:	2016-325T00:01:45.607	Stop Time:	2016-325T23:58:16.055
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016326_01

Start Time:	2016-326T00:00:16.054	Stop Time:	2016-326T23:57:07.979
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_2016327_01

Start Time:	2016-327T00:01:24.590	Stop Time:	2016-327T23:58:22.073
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016328_01

Start Time:	2016-328T00:01:22.072	Stop Time:	2016-328T23:59:52.520
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016329_01

Start Time:	2016-329T00:02:52.519	Stop Time:	2016-329T23:59:51.967
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016330_01

Start Time:	2016-330T00:02:51.965	Stop Time:	2016-330T23:57:22.414
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016331_01

Start Time:	2016-331T00:00:22.413	Stop Time:	2016-331T23:57:22.861
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016332_01

Start Time:	2016-332T00:00:22.860	Stop Time:	2016-332T23:59:51.245
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_2016333_01

Start Time:	2016-333T00:04:06.048	Stop Time:	2016-333T23:59:07.719
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016334_01

Start Time:	2016-334T00:03:23.300	Stop Time:	2016-334T23:59:44.076
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016335_01

Start Time:	2016-335T00:01:44.075	Stop Time:	2016-335T23:59:53.226
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016336_01

Start Time:	2016-336T00:04:08.584	Stop Time:	2016-336T23:58:48.033
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016337_01

Start Time:	2016-337T00:03:05.640	Stop Time:	2016-337T23:57:04.543
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016338_01

Start Time:	2016-338T00:00:04.542	Stop Time:	2016-338T23:57:04.990
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016339_01

Start Time:	2016-339T00:00:04.988	Stop Time:	2016-339T23:56:33.206
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016340_01

Start Time:	2016-340T00:00:48.400	Stop Time:	2016-340T23:59:57.882
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016341_01

Start Time:	2016-341T00:02:57.881	Stop Time:	2016-341T23:58:58.329
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016342_01

Start Time:	2016-342T00:01:58.328	Stop Time:	2016-342T23:58:58.776
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016343_01

Start Time:	2016-343T00:01:58.775	Stop Time:	2016-343T23:58:58.223
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_2016344_01

Start Time:	2016-344T00:01:58.222	Stop Time:	2016-344T23:58:58.670
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016345_01

Start Time:	2016-345T00:01:58.669	Stop Time:	2016-345T23:58:49.859
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016346_01

Start Time:	2016-346T00:02:29.116	Stop Time:	2016-346T23:59:59.563
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016347_01

Start Time:	2016-347T00:02:59.562	Stop Time:	2016-347T23:57:00.011
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_2016348_01

Start Time:	2016-348T00:00:00.010	Stop Time:	2016-348T23:57:43.396
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_2016349_01

Start Time:	2016-349T00:02:00.988	Stop Time:	2016-349T23:57:01.905
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_2016350_01

Start Time:	2016-350T00:00:01.904	Stop Time:	2016-350T23:57:02.352
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016351_01

Start Time:	2016-351T00:00:02.351	Stop Time:	2016-351T23:57:01.798
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016352_01

Start Time:	2016-352T00:00:01.797	Stop Time:	2016-352T23:57:02.245
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_2016353_01

Start Time:	2016-353T00:00:02.244	Stop Time:	2016-353T23:59:32.691
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_2016354_01

Start Time:	2016-354T00:02:32.690	Stop Time:	2016-354T23:57:33.138
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016355_01

Start Time:	2016-355T00:00:33.137	Stop Time:	2016-355T23:59:03.585
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_2016356_01

Start Time:	2016-356T00:02:03.583	Stop Time:	2016-356T23:58:35.032
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016357_01

Start Time:	2016-357T00:01:35.031	Stop Time:	2016-357T23:57:04.479
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016358_01

Start Time:	2016-358T00:00:04.478	Stop Time:	2016-358T23:59:35.925
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016359_01

Start Time:	2016-359T00:02:35.924	Stop Time:	2016-359T23:59:35.372
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016360_01

Start Time:	2016-360T00:02:35.371	Stop Time:	2016-360T23:59:06.757
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016361_01

Start Time:	2016-361T00:01:36.756	Stop Time:	2016-361T23:59:09.141
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016362_01

Start Time:	2016-362T00:01:09.140	Stop Time:	2016-362T23:57:07.714
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016363_01

Start Time:	2016-363T00:00:07.712	Stop Time:	2016-363T23:57:08.160
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016364_01

Start Time:	2016-364T00:00:08.159	Stop Time:	2016-364T23:57:08.607
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

CMFULL0_2016365_01

Start Time:	2016-365T00:00:08.606	Stop Time:	2016-365T23:57:09.054
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_2016366_01

Start Time:	2016-366T00:00:09.053	Stop Time:	2016-366T23:57:08.501
Chems full time resolution intensities for all CHEMS rate channels for which efficiencies are also known. Some CHEMS rate channels can only be calibrated to counts/sec, but these channels can be and have been convereted to particle intensities. In some cases, efficiencies for lower DPPS steps are too low to be useful, and so that steps are not included in the spectra. These channels have better statistics than the PHA channels, but have more issues with backgrounds. The MIMI User's Guide has more details on these channels. Following the data are columns describing certain geometric parameters such as the position of Cassini in the SZS and SZO frames. Also included are the pitch angles of the CHEMS telescopes, and the exact time of observation for each particular dpps step in a row of data.

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