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Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
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木星の上層大気の熱構造は,ガリレオ探査機から得られたものです

Seiff1, Kirk, Knight

  • 1A. Seiff, Department of Meteorology, San Jose State University Foundation and MS 245-1, Ames Research Center, Moffett Field, CA 94035, USA. D. B. Kirk, University of Oregon, 37465 Riverside Drive, Pleasant Hill, Oregon 97455, USA. T. C. D. Knight, 2370 S. Brentwood St., Lakewood, CO 80227, USA. L. A. Young, Center for Space Physics, Boston University, 725 Commonwealth Ave., Boston, Massachusetts 02215, USA. F. S. Milos, M.S. 234-1, Ames Research Center, NASA, Moffett Field, CA 94035, USA. E. Venkatapathy, Eloret Institute, MS 230-2, Ames Research Center, Moffett Field, CA 94035, USA. J. D. Mihalov and R. E. Young, MS 245-3, Ames Research Center, Moffett Field, CA 94035, USA. R. C. Blanchard, MS 408A, Langley Research Center, NASA, Hampton, VA 23681, USA. G. Schubert, Department of Earth and Space Sciences, University of California, Los Angeles, CA 90024, USA.

Science (New York, N.Y.)
|April 4, 1997
PubMed
まとめ

木星の大気は高度に大きく加熱され,頂点付近で900ケルビンに達します. 波のような振動と波のエネルギー消耗が,この上層大気の加熱の原因である可能性が高い.

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