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Updated: Jul 12, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
07:17

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry

Published on: August 1, 2017

コメット・ジャコビニ・ジンナー: プラズマ説明

S J Bame, R C Anderson, J R Asbridge

    Science (New York, N.Y.)
    |April 18, 1986
    PubMed
    まとめ

    国際彗星探査機 (ICE) は,強烈な太陽風の相互作用を彗星ジャコビニ・ジンナーと観測した. 弓の衝撃は検出されなかったが,移行領域,シート,およびプラズマの尾が特定され,複雑な彗星のプラズマダイナミクスを明らかにした.

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