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木星の磁気圏におけるコロテーション・ラグ:観測と理論の比較

T W Hill

    Science (New York, N.Y.)
    |January 18, 1980
    PubMed
    まとめ

    ヴォイジャー1号のデータは,木星の磁気圏のコロテーション遅延を説明する理論を裏付けている. この遅延は,急速なプラズマ生成と弱い大気と磁気圏の結合により発生し,当初予想よりも高いプラズマ生成率を必要とします.

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