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タイタンの中緯度の雲の進化

C A Griffith1, P Penteado, K Baines

  • 1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.

Science (New York, N.Y.)
|October 22, 2005
PubMed
まとめ

タイタンの雲はダイナミックで,コンベクティブプロセスや雨によって急速に形成され,散らばります. これらの雲の動態は,大気循環と土星の月の表面力によって影響を受けます.

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