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Titan's hydrodynamically escaping atmosphere: Escape rates and the structure of the exobase region

✍ Scribed by Darrell F. Strobel


Book ID
103830523
Publisher
Elsevier Science
Year
2009
Tongue
English
Weight
538 KB
Volume
202
Category
Article
ISSN
0019-1035

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As on Earth, Titan's atmosphere plays a major role in the cooling of heated surfaces. We have assessed the mechanisms by which Titan's atmosphere, dominantly N 2 at a surface pressure of 1.5 Γ‚ 10 5 Pa, cools a warm or heated surface. These heated areas can be caused by impacts generating melt sheets