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アルフヴェン波の証拠は太陽のX線ジェットにある

J W Cirtain1, L Golub, L Lundquist

  • 1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. Jonathan.W.Cirtain@nasa.gov

Science (New York, N.Y.)
|December 8, 2007
PubMed
まとめ

新しい観測により,極の冠状孔から発生する多数の高速X線ジェットが明らかになった. これらのダイナミックなイベントは,頻繁に発生し,高速太陽風に大きく寄与する可能性があります.

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