@inproceedings{e88e842f0dcd44a29e7ca280bf3bd455,
title = "Global mapping of Titan in the infrared using a heuristic approach to reduce the atmospheric scattering component",
abstract = "Titan is the largest satellite of Saturn, and the only one to have a dense atmosphere. Whereas its surface cannot be seen at visible wavelengths due to the strong absorption and scattering of the atmospheric gases (mainly N2 and CH4) and aerosols, it can be seen at specific wavelengths in the infrared. We focus in this paper on the global mapping of Titan geological units using the Visual and Infrared Mapping Spectrometer onboard Cassini, and discuss the problem of the decorrelation between atmospheric and surface components.",
keywords = "Cassini, Hyperspectral, Infrared, Titan, VIMS",
author = "{Le Mou{\'e}lic}, S. and T. Cornet and S. Rodriguez and C. Sotin and Barnes, {J. W.} and Brown, {R. H.} and O. Bourgeois and Baines, {K. H.} and Buratti, {B. J.} and Clark, {R. N.} and Nicholson, {P. D.}",
year = "2010",
doi = "10.1109/WHISPERS.2010.5594903",
language = "English (US)",
isbn = "9781424489077",
series = "2nd Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2010 - Workshop Program",
booktitle = "2nd Workshop on Hyperspectral Image and Signal Processing",
note = "2nd Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2010 ; Conference date: 14-06-2010 Through 16-06-2010",
}