| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8144226 | Planetary and Space Science | 2012 | 14 Pages |
Abstract
⺠Huygens-DISR measured Titan's surface reflectivity using the Surface Science Lamp. ⺠The phase curve between 0.02° and 80° phase angle suggests a strong opposition surge. ⺠The reflectivity spectrum is smooth, peaking at 0.45 at 750 nm wavelength, 0° phase. ⺠The probed terrain within 100 m of the landing site is very homogeneous. ⺠The methane mixing ratio of the atmosphere near the surface is 5.0±0.3%.
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Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Erich Karkoschka, Stefan E. Schröder, Martin G. Tomasko, Horst Uwe Keller,