| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8144194 | Planetary and Space Science | 2012 | 10 Pages |
Abstract
⺠Global surface mapping of Titan using visible wavelength channels from Cassini VIMS. ⺠Methane windows at 0.637, 0.681, 0.754, 0.827, 0.937, and 1.046μm. ⺠The first global surface reflectance maps of Titan shortward of 0.938μm. ⺠We employ an empirically derived algorithm to remove haze layers from Titan.
Related Topics
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Earth and Planetary Sciences
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Authors
Graham Vixie, Jason W. Barnes, Jacob Bow, Stéphane Le Mouélic, Sébastien Rodriguez, Robert H. Brown, Priscilla Cerroni, Federico Tosi, Bonnie Buratti, Christophe Sotin, Gianrico Filacchione, Fabrizio Capaccioni, Angioletta Coradini,