Titan Surface-Atmospheric Separation Models For Cassini VIMS: Spherical-Shell Radiative Transfer Models

Details Titan Surface-Atmospheric Separation Models For Cassini VIMS: Spherical-Shell Radiative Transfer Models Titan Surface-Atmospheric Separation Models For Cassini VIMS: Spherical-Shell Radiative Transfer Models

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1911p&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

1

Scientific paper

We explore the utility of 2D spherical-shell radiative transfer codes
for Cassini Visual and Infrared Mapping Spectrometer I/F data that cover
a range of latitude and longitude coordinates and incorporate recently
released Titan atmospheric structure data from Huygens DISR.

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