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Updated: Aug 1, 2026

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木星の大気の構造:ガリレオ探査機の測定結果

Seiff1, Kirk, Knight

  • 1A. Seiff, Department of Meteorology, San Jose State University, San Jose, CA 95192, USA. D. B. Kirk, 37465 Riverside Drive, Pleasant Hill, OR 97455, USA. T. C. D. Knight, 2370 South Brentwood Street, Lakewood, CO 80227, USA. J. D. Mihalov, R. E. Young, F. S. Milos, J. Wang, NASA Ames Research Center, Moffett Field, CA 94035, USA. R. C. Blanchard, NASA Langley Research Center, Hampton, VA 23681, USA. G. Schubert, Department of Earth and Space Science, University of California, Los Angeles, CA 90024, USA. U. von Zahn, Institut fur Atmospharenphysik, Universitat Rostock, D(0)-2565 Kuhlungsborn, Germany. G. Lehmacher, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.

Science (New York, N.Y.)
|May 10, 1996
PubMed
まとめ

ガリレオ探査機のデータは,木星の大気には深い水の雲がなく,乾燥したアディアバットに続く温度を示しています. 上層大気分析は,熱いエクソスフィアと鋭い熱グラデーションを確認しています.

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