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Updated: Apr 27, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
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宇宙の天気,宇宙の天気 マグネトテイル再接続のアイオノスフィアの制御

William Lotko1, Ryan H Smith2, Binzheng Zhang2

  • 1Thayer School of Engineering, Dartmouth College, Hanover, NH, USA. Research Affiliate, High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA. wlotko@dartmouth.edu.

Science (New York, N.Y.)
|July 12, 2014
PubMed
まとめ

地球の磁気尾の高速プラズマフローは,磁気再接続により,夜前セクターに集中しています. グローバルシミュレーションでは,ホール伝導度グラデーションによって引き起こされるイオン圏-磁気圏の相互作用が,観測されたこの非対称性を引き起こしていることが明らかになっています.

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