Global-scale surface spectral variations on Titan seen from Cassini/VIMS
By Jason W. Barnes, Robert H. Brown, L. Soderblom, B. Buratti, Christophe Sotin, S. Rodriguez, S. Mouélic, K. Baines, R. Clark, P. Nicholson. 2007
134 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/d0790fef5a95cb263d506a657e254e96c2e8a00d
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In Astronomy and Astrophysics
Citations in the corpus
- Cryovolcanism on Titan: New results from Cassini RADAR and VIMS (2013, methodology): “[43] Hotei Regio is unusually bright at 5mm [Barnes et al., 2005], similar to Tui Regio (see next section). SAR images revealed lobate features that form radar-bright and radar-dark patterns.Wall et al. [2009] interpreted the radar-bright features as likely cryovolcanic in origin. However, when topo”
- Spectroscopy, morphometry, and photoclinometry of Titan's dunefields from Cassini/VIMS (2008, methodology): “…calling the areas “sand” is arbitrary Near the west end of the swath, at 15.9 ◦ N 63.2 ◦ W, is an outcrop of the equatorial bright spectral unit [as described in Barnes et al. (2007a); this unit corresponds to the bright neutral unit from Soderblom et al. (2007) near the equator] 5–10 km across .”