,

Chuan-Yi Tu1, Cheng Zhou, Eckart Marsch

  • 1Department of Geophysics, Peking University, Beijing 100871, China. cytu@public3.bta.net.cn

Science (New York, N.Y.)
|April 23, 2005
PubMed
まとめ

太陽風は,太陽の冠状孔から発生し,磁気フンネル内の光球より5〜20メガメートルの高さから流出を開始します. この発見は,太陽風の現象を明確にしています.

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