Surface-Atmosphere Interaction on Titan : Cassini RADAR Results

Details Surface-Atmosphere Interaction on Titan : Cassini RADAR Results Surface-Atmosphere Interaction on Titan : Cassini RADAR Results

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007epsc.conf..610l&link_type=abstract

European Planetary Science Congress 2007, Proceedings of a conference held 20-24 August, 2007 in Potsdam, Germany. Online at ht

Physics

Scientific paper

Titan's surface is intimately connected with the atmosphere, and the Cassini RADAR investigation reveals many aspects of this interaction. Examples include fluvial channels indicative of methane rainstorms, sand dunes shaped by possibly tidal winds, and polar lakes. Some recent results from Radar imaging of Titan's landscape, as well as nonimaging results (topography, radiometry etc.) will be summarized.

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