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深いメリディアン流の太陽斑の緯度分布を説明する

Dibyendu Nandy1, Arnab Rai Choudhuri

  • 1Department of Physics, Indian Institute of Science, Bangalore 560012, India. dandy@physics.iisc.ernet.in

Science (New York, N.Y.)
|June 1, 2002
PubMed
まとめ

新しい太陽ダイナモモデルでは,コンベクションゾーンの下に浸透する深度のメリディアン流により,低緯度で太陽斑が形成されていることが示されています. この発見は,以前のモデルに異議を唱え,太陽物理学にも影響を及ぼしている.

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