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Giant Molecular Cloud Formation through the Parker Instability in a Skewed Magnetic Field 

作成者 松元, 亮治
キーワード等 hydromagnetics, instabilities, interstellar, magnetic fields
日本十進分類法 (NDC) 440
内容 The effect of the magnetic skew on the Parker instability is investigated bymeans of the linear stability analysis for a gravitationally stratied gas layer permeatedby a horizontal magnetic eld. When the magnetic eld is skewed (i.e., theeld line direction is a function of the height), the wavelength of the most unstablemode is 10H where H is the pressure scale height. The growth rate of theshort wavelength modes is greatly reduced when the gradient in the magnetic elddirection exceeds 0.5 radian per scale height. Our results indicate that the Parkerinstability in a skewed magnetic eld preferentially forms large scale structures likegiant molecular clouds.
作成日付 1995-05
コンテンツの種類 プレプリント Preprint
DCMI資源タイプ text
ファイル形式 applicaiton/pdf
ハンドルURL http://mitizane.ll.chiba-u.jp/meta-bin/mt-pdetail.cgi?cd=00020208
フルテキストへのリンク http://mitizane.ll.chiba-u.jp/metadb/up/joho/matsumoto_9205002X.pdf
言語 英語


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hydromagnetics
instabilities
interstellar
magnetic fields