6. 太陽プラズマにおけるMHD (<講座>MHDモデルと磁気核融合V)

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概要

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• MHD approaches adopted in the cosmical plasma problems turn out to be very productive, though there are, of course, types of problems in which they have limitation for the application. Here, we deal with the MHD problems in the solar atmosphere which is a "show case" of the general cosmic plasma problems with greater scales. The solar X-ray satellite "Yohkoh", having high resolution telescopes in the soft and hard X-ray ranges observing the Sun with high cadence, has revealed a very dynamic behavior of the high temperature atmosphere, the corona, and revealed essential clues including those of the yet fainter stages in various types of violent phenomena occurring in it. We here describe those new developments in this field that provide us with the basis for the more general cosmic plasmadynamical phenomena including stellar and galactic magnetic activity.

• 社団法人プラズマ・核融合学会の論文
• 1995-08-25

著者

• 内田 豊

  東京理科大学・理学部

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• 6. 太陽プラズマにおけるMHD (MHDモデルと磁気核融合V)

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