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Cassini High Rate Detector V14.0
Economou, T.; DiDonna, P.
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 December 31, 2013. Please refer to Srama et al. (2004) for a det…
Gaskell Dione Shape Model V1.0
Gaskell, R. W.
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.
Gaskell Mimas Shape Model V2.0
Gaskell, R. W.
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.
Cassini High Rate Detector V12.0
Economou, T.; DiDonna, P.
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 December 31, 2012. Please refer to Srama et al. (2004) for a det…
Gaskell Tethys Shape Model V1.0
Gaskell, R. W.
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.
Mimas Shape Model V1.0
Gaskell, R. W.
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA 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 July 14, 2010. Vertex-facet versions of the models are also provided.
Phoebe Shape Model V1.0
Gaskell, R. W.
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 July 7, 2010. Vertex-facet versions of the models are also provided.
Ulysses Dust Detection System V3.1
Dikarev, V.; Srama, R.; Hamilton, D. P. +26 more
This data set contains the data from the Ulysses dust detector system (UDDS) from start of mission through the end of mission, 1990-2007. (As the dust detector was turned off after Nov. 30, 2007, this is the last date for which UDDS data is recorded.) Included are the dust impact data, noise data, laboratory calibration data, and location and orie…
Cassini Cosmic Dust Analyser Data V1.0
Kempf, S.; Srama, R.; Altobelli, N.
The Cosmic Dust Analyzer (CDA) is an instrument on the Cassini Orbiter that studies the physical properties of dust particles hitting the detector. This data set includes all data from the CDA with the exception of the High Rate Detector (HRD).
Small Main-belt Asteroid Spectroscopic Survey, Phase II
Binzel, R. P.; Bus, S.
This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure o…