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Updated: Jul 12, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
06:42

Magnetically Induced Rotating Rayleigh-Taylor Instability

Published on: March 3, 2017

急速回転する巨大惑星のモデルにおいて,コンベクションによって維持される帯状の表面流動

Z P Sun, G Schubert, G A Glatzmaier

    Science (New York, N.Y.)
    |April 30, 1993
    PubMed
    まとめ

    回転する流体殻の熱的に駆動されたコンベクションは,惑星の大気を模倣した帯状のゾーン流を生み出します. これらのシミュレーションは,木星と土星の原因として,コンベクションを支持しています.

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