Global mapping of Titan at 2-cm wavelength

Details Global mapping of Titan at 2-cm wavelength Global mapping of Titan at 2-cm wavelength

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufm.p33e..03j&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #P33E-03

Physics

[6281] Planetary Sciences: Solar System Objects / Titan, [6969] Radio Science / Remote Sensing

Scientific paper

Six years of radiometric observations of Titan using the radiometric capability of the Cassini RADAR instrument have been reduced to provide global maps of thermophysical properties of Titan’s surface, including radiometric brightness, emissivity, effective dielectric constant, and volume scattering from the subsurface. These maps provide a unique insight into such surface properties as overall composition and structure on wavelength scales. Geophysical implications will be discussed. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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