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Updated: Aug 18, 2026

Three-dimensional Particle Tracking Velocimetry for Turbulence Applications: Case of a Jet Flow
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木星における浸透的コンベクションとゾーンフロー

Zhang1, Schubert

  • 1K. Zhang, Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA, and Department of Mathematics, University of Exeter, Exeter, EX4 4QJ, UK. G. Schubert, Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angeles, CA 90095, USA.

Science (New York, N.Y.)
|August 16, 1996
PubMed
まとめ

木星の内部にある深層のコンベクションは,大気風を駆動する可能性があります. 回転効果により,このコンベクションが外層に浸透し,木星で観測されたゾナルの風パターンを発生させます.

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