Search Results

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Data Sets and Information
• bundle: Saturn Zonal Winds Bundle
  Saturn's zonal wind profile in 2004-2009 from Cassini ISS images
• bundle: Cassini Orbiter RSS Neutral Atmosphere T-P profiles for Titan Bundle
  Atmospheric profiles of Titan
• bundle: Titan Ionosphere Bundle
  Cassini radio occultations of the Titan ionosphere
• bundle: 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.
• bundle: Cassini Orbiter Radio Science Subsystem Occultation and Electron Density
  Derived data products from Cassini radio occultations at Titan and their accompanying documentation. Derived data products include: (A) time series of the frequency of the radio signal received at Earth during an occultation; (B) individual electron density profiles from occultations; (C) average electron density profiles from occultations; and (D) summary of average electron density profiles.
• bundle: Saturn Ionosphere Bundle
  Cassini radio occultations of the Saturn ionosphere
• bundle: 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.
• bundle: 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.
• bundle: 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.
• bundle: 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.
• bundle: 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.
• bundle: 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.
• bundle: 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.
• bundle: 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.
• bundle: C2H4 mole fraction and temperature profiles after the 2010 Saturn Storm
  Mole fractions during the 2010 Saturn Storm
• bundle: 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.
• bundle: Cassini RPWS Electron Densities from Upper Hybrid and Plasma Wave Frequencies
  This bundle provides electron number density values derived from features observed in plasma wave data obtained by the Cassini Radio and Plasma Wave Science (RPWS) instruments, along with observed or derived characteristic frequencies, and useful positional parameters for the spacecraft and related bodies. When present, frequency values of narrowband emissions at the upper hybrid resonance were digitized and combined with measured or model magnetic field to derive electron number density. At other times, features such as the upper cutoff in auroral hiss or electron plasma oscillations were used to determine the plasma frequency and electron density.
• bundle: Cassini CAPS Fitted Parameters Bundle
  This data set consists of all of the fits (both good and bad) that were found by Dr. Robert J. Wilson during the NASA Cassini Data Analysis Program grant (NNX12AG90G). The Cassini CAPS plasma data used in the forward model plasma parameter calculations given here came from volume CO-E/J/S/SW-CAPS-2-UNCALIBRATED-V1.0 in the Planetary Data System (PDS).