Data Set Information
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| DATA_SET_NAME |
CASSINI ORBITER SATURN UVIS STELLAR RING OCC 2004-2017
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| DATA_SET_ID |
CO-SR-UVIS-2/4-OCC-V2.0
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| NSSDC_DATA_SET_ID |
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| DATA_SET_TERSE_DESCRIPTION |
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| DATA_SET_DESCRIPTION |
Data Set Overview: This data set contains derived radial occultation profiles of the rings of Saturn based on stellar occultation observations made with the Cassini UVIS instrument between October 2004 and August 2017. Version 1.0 Contains derived radial occultation profiles of the rings of Saturn based on stellar occultation observations made with the Cassini UVIS instrument between May 2005 and August 2008. Version 2.0 Contains derived radial occultation profiles of the rings of Saturn based on stellar occultation observations made with the Cassini UVIS instrument between October 2004 and August 2017. Geometric calculations were based on the final (post mission) NAIF kernel files. All previously archived profiles were reprocessed for inclusion in the Version 2.0 delivery. With version 2.0, the columns in the data table files were reordered slightly, and an additional column, OBSERVED RING AZIMUTH, was added. Definitions of all of the ring specific keywords and columns may be found in Occultation_keywords_v1.3.pdf in the document subdirectory. Added additional documentation files.Processing: High. Limitations encountered in the data and the processing are detailed in Colwell etal. 2010 (COLWELLETAL2010).
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| DATA_SET_RELEASE_DATE |
2019-05-03T00:00:00.000Z
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| START_TIME |
2004-10-06T04:33:30.000Z
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| STOP_TIME |
2017-08-16T06:35:55.000Z
|
| MISSION_NAME |
CASSINI-HUYGENS
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| MISSION_START_DATE |
1997-10-15T12:00:00.000Z
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| MISSION_STOP_DATE |
2017-09-15T12:00:00.000Z
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| TARGET_NAME |
S RINGS
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| TARGET_TYPE |
RING
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| INSTRUMENT_HOST_ID |
CO
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| INSTRUMENT_NAME |
ULTRAVIOLET IMAGING SPECTROGRAPH
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| INSTRUMENT_ID |
UVIS
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| INSTRUMENT_TYPE |
SPECTROGRAPH
|
| NODE_NAME |
Planetary Rings
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| ARCHIVE_STATUS |
SUPERSEDED
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| CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview: The data have been processed and reviewed by members of the UVIS team. Limitations encountered in the data and the processing are detailed in Colwell etal. 2010 (COLWELLETAL2010).Review: This data set has completed a PDS Peer Review.Contact Information: For questions concerning this data set contact: Mitch Gordon PDS Rings Node SETI Institute 189 Bernardo Ave. Mountain View, CA 94043 Phone: 276-393-8822 Email: mgordon@seti.org Josh Colwell University of Central Florida Department of Physics 4000 Central Florida Blvd Orlando, FL 32816-2385 Phone: 407-823-2012 Email: jcolwell@physics.ucf.edu
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| CITATION_DESCRIPTION |
Colwell, J.E., R.G. Jerousek, T.M. Becker, and L.W. Esposito, CASSINI ORBITER SATURN UVIS RING STELLAR OCCULTATIONS 2.0, CO-SR-UVIS-HSP-2/4-OCC-V2.0, NASA Planetary Data System, 2019.
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| ABSTRACT_TEXT |
This data set contains derived radial occultation profiles of the rings of Saturn based on stellar occultation observations made with the Cassini UVIS instrument between October 2004 and August 2017.
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| PRODUCER_FULL_NAME |
MITCHELL K. GORDON
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| SEARCH/ACCESS DATA |
Rings Node Interface
Rings Online Archives
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