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.

This data set contains derived
radial occultation profiles of the rings of Saturn based on stellar
occultations made with the Cassini VIMS instrument during the Cassini
nominal mission.

This data set comprises uncalibrated
and calibrated data from the Cassini Composite Infrared Spectrometer
(CIRS) instrument. The basic data is comprised of uncalibrated raw spectra,
along with along with pointing and geometry information, and
housekeeping information. Also included are calibrated power spectra,
and documentation.

This data set contains calibrated full time resolution Cassini magnetometer data, for the entire Cassini mission. These data are provided in RTN coordinates for cruise, and Kronographic (KRTP) coordinates for Saturn Tour. They have been calibrated and converted to physical coordinates from the Cassini MAG Raw Data Set (CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0), by the Cassini MAG team at Imperial College.

This data set contains derived
radial occultation profiles of the rings of Saturn based on stellar
occultations made with the Cassini VIMS instrument during the Cassini
nominal mission.

This data set contains derived
radial occultation profiles of the rings of Saturn based on radio
occultations made with the Cassini RSS instrument during the Cassini
nominal mission.

This data set contains calibrated 1 second averaged Cassini magnetometer data, for the entire Cassini mission. These data are provided in Kronographic (KRTP, KSO, KSM) coordinates at Saturn, Geographic coordinates (GSE, GSM) for the Earth flyby, Jovigraphic coordinates for the Jupiter flyby, and RTN coordinates for the entire mission. These data were calibrated and converted to physical coordinates from the Cassini MAG Raw Data Set (CO-E/SW/J/S-MAG-2-REDR-RAW-DATA-V1.0), by the Cassini MAG team at Imperial College. The data averaged to 1 second at the PDS-PPI node at UCLA.

This data set contains calibrated 1 minute averaged Cassini magnetometer data, for the entire Cassini mission. These data are provided in Kronographic (KRTP, KSO, KSM) coordinates at Saturn, Geographic coordinates (GSE, GSM) for the Earth flyby, Jovigraphic coordinates for the Jupiter flyby, and RTN coordinates for the entire mission. These data were calibrated, converted to physical coordinates and averaged to 1 minute by the Cassini MAG team at Imperial College.

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.

The Cassini Radio Science Saturn Gravity and Ring Occultation experiments (SAGR19) Raw Data Archive is a time-ordered collection of radio science raw data acquired on July 18 and 19, 2017, during the Cassini Extended Extended Mission.