Search Results
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Quasi Thermal Noise pectroscopy on High Frequency Receiver Data Bundle
This bundle contains RPWS-HFR Quasi Thermal Noise (QTN) spectroscopy supplied CDF and plot files containing a time series of thermal plasma moments (density and temperature). QTN data products are generated only when the QTN analysis is applicable. -
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VIMS Observations from the Cassini Cruise to Saturn
This bundle contains Cassini VIMS data, metadata, and associated documentation from the cruise to Saturn--October 1997 through December 2003. -
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Arizona State University Ronald Greeley Center for Planetary Studies - The Ronald Greeley 35mm Slide Collection, The Jovian System
This bundle contains the digitized products generated from Dr. Ronald Greeley's 35mm Slide Collection, the Jovian System, housed at the RGCPS, ASU, Tempe, AZ. Included is a User’s Guide for a further description of the products. -
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VIMS Observations from the Cassini Tour of the Saturn System
This bundle contains Cassini VIMS data, metadata, and associated documentation for the Saturn tour--January 2004 through end of mission in September 2017. -
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GASKELL DIONE SHAPE MODEL
The shape model of Dione derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 23, 2012. Vertex-facet versions of the models are also provided. -
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GASKELL MIMAS SHAPE MODEL
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA and ISSWA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on June 26, 2012. Vertex-facet versions of the models are also provided. -
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Cassini MIMI CHEMS Raw Bundle
This bundle contains Cassini Magnetospheric Imaging Instrument (MIMI) Charge Energy Mass Spectrometer (CHEMS) accumulation, pulse height analysis and science rate data for 1999-01-03T00:00:00Z to 2017-09-15T23:59:59Z. -
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ISS Observations from the Cassini Cruise to Saturn
This bundle contains Cassini ISS images, metadata, and associated documentation from the cruise to Saturn--October 1997 through December 2003. -
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GASKELL PHOEBE SHAPE MODEL
The shape model of Phoebe derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on August 4, 2012. Vertex-facet versions of the models are also provided. -
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Cassini MIMI INCA Raw Bundle
This bundle contains Cassini Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) accumulation, images and pulse height analysis data for 1999-01-03T00:00:00.000Z to 2017-09-15T23:59:59.000Z. -
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Saturn Ring System Solar Occultations Observed by Cassini UVIS
This bundle contains derived time series data products from multiple solar occultations by the rings of Saturn. -
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ISS Observations from the Cassini Tour of the Saturn System
This bundle contains Cassini ISS images, metadata, and associated documentation for the Saturn tour--January 2004 through end of mission in September 2017. -
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CASSINI HIGH RATE DETECTOR
The High Rate Detector (HRD) from the University of Chicago is an independent part of the CDA instrument on the Cassini Orbiter that measures the dust flux and particle mass distribution of dust particles hitting the HRD detectors. This data set includes all data from the HRD through the end of the mission, Sept. 15, 2017. Please refer to Srama et al. (2004) for a detailed HRD description. -
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GASKELL TETHYS SHAPE MODEL
The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012. Vertex-facet versions of the models are also provided. -
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Saturn Small Moon Shape Models V1.0
Digital shape models have been constructed from Cassini Imaging Science Subsystem (ISS) data for eleven of the small satellites of Saturn and delivered to the Planetary Data System. These satellites are: Pan, Daphnis, Atlas, Prometheus, Pandora, Epimetheus, Janus, Telesto, Calypso, Helene, and Hyperion. These models typically have uncertainties well under 0.5 km. They are appropriate for global geometric, geologic, and geophysical studies, and regional slope and topography study. They are useful in studying morphologies of only the relatively largest-sized craters. Studies based on early versions of these shape models are in Thomas et al., 2013 -
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Phoebe SPC Shape Model and Assessment Products V1.0
This bundle contains a shape model for the Saturnian moon Phoebe, along with quality assessment data. The global model is similar to the previously archived "Gaskell Phoebe Shape Model", but is provided in multiple formats.
Data Sets and Information