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Updated: Jul 12, 2026

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation
08:36

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation

Published on: November 3, 2016

密度の高い天体物理プラズマである

H M VAN Horn

    Science (New York, N.Y.)
    |April 19, 1991
    PubMed
    まとめ

    この研究は,巨大惑星,茶色矮星,白矮星,中性子星などの天体のモデリングに不可欠な,密度の高いプラズマの物理的特性を探求しています. これらの性質を理解することは,天体物理学と恒星の進化理論の進歩の鍵です.

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