Global Mapping of Titan in the Infrared Using an Empirical Decorrelation Between Atmosphere and Surface

Details Global Mapping of Titan in the Infrared Using an Empirical Decorrelation Between Atmosphere and Surface Global Mapping of Titan in the Infrared Using an Empirical Decorrelation Between Atmosphere and Surface

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1730l&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 present an empirical approach to decorrelate surface and atmospheric
(additive and multiplicative) contributions in VIMS infrared spectral
images of Titan. The aim is to produce homogenized global mosaics of the
main surface units of Titan.

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