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Updated: May 2, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
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潮の消散と地球の内部磁場の強さ

Bruce A Buffett1

  • 1Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA. bbuffett@berkeley.edu

Nature
|December 18, 2010
PubMed
まとめ

この研究は,潮分散測定を用いて地球の内部磁場強さを推定しています. 2.5ミリテスラ (mT) のコア平均フィールドは,地球のニュテーションにおける観測された異常を説明し,ジオダイナモの電力要求を制限します.

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