Mapping Titan's surface features within the visible spectrum via Cassini VIMS-Reference-Cited by-同舟云学术

Mapping Titan's surface features within the visible spectrum via Cassini VIMS

Published:2012-01 Issue:1 Volume:60 Page:52-61
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Vixie Graham,Barnes Jason W.,Bow Jacob,Le Mouélic Stéphane,Rodriguez Sébastien,Brown Robert H.,Cerroni Priscilla,Tosi Federico,Buratti Bonnie,Sotin Christophe,Filacchione Gianrico,Capaccioni Fabrizio,Coradini Angioletta

Funder

NASA Outer Planets Research program

ASI

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

1. Cassini observations of flow-like features in western Tui Regio, Titan;Barnes;Geophysical Research Letters,2006

2. Global-scale surface spectral variations on Titan seen from Cassini/VIMS;Barnes;Icarus,2007

3. A 5-micron-bright spot on Titan: evidence for surface diversity;Barnes;Science,2005

4. VIMS spectral mapping observations of Titan during the Cassini prime mission;Barnes;Planetary and Space Science,2009

5. The Cassini Visual and Infrared Mapping Spectrometer (VIMS) investigation;Brown;Space Science Reviews,2004

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