Spectroscopic investigation of Dione' surface using Cassini VIMS images

Details Spectroscopic investigation of Dione' surface using Cassini VIMS images Spectroscopic investigation of Dione' surface using Cassini VIMS images

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..474s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.474

Physics

Scientific paper

Dione was observed several times by the Cassini spacecraft in its nominal and extended mission from 2004 to 2010. We have selected 76 Cassini/VIMS hyperspectral cubes of Dione in the IR range between 0.85 and 5.1 μm and we have applied the Spectral Angle Mapper (SAM) clustering technique to classify different surface units on the basis of their spectral properties. We identify nine different terrain types correlated to specific Dione' surface morphologies.

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