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太陽染色球の闇の中心に新しい光が照らされる

S K Solanki, W Livingston, T Ayres

    Science (New York, N.Y.)
    |January 7, 1994
    PubMed
    まとめ

    太陽染色体の冷たい成分である3500Kは,一酸化炭素のスペクトルを用いて検出されています. このコンポーネントは,静かな太陽表面のほとんどをカバーし,ガス膨張に関連しています.

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