Investigating the Surface of Titan in the 1-2.8 µm Range with CassiniI/VIMS Hyperspectral Images

Details Investigating the Surface of Titan in the 1-2.8 µm Range with CassiniI/VIMS Hyperspectral Images Investigating the Surface of Titan in the 1-2.8 µm Range with CassiniI/VIMS Hyperspectral Images

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1745l&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1745

Physics

Scientific paper

We focus in this presentation on the global mapping of the surface of
Titan using data from the Visual and Infrared Mapping Spectrometer
(VIMS) onboard Cassini. The objective is to produce seamless mosaics in
the short-wavelength surface windows.

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