Observational Constraint to the Minimum Flux Corona Model

スポンサーリンク

概要

• 論文の詳細を見る

• The minimum flux corona model proposed by Hearn was compared with the observational data. The temperature derived from Hearn's model is lower than that derived from X-ray observation for latetype main-sequence stars. In the solar coronal hole, Hearn's minimum condition is not realized. The minimum flux corona model seems to be adequate only to the solar quiet region.Minimum flux corona modelSolar coronaStellar corona

• 東北大学の論文
• 1985-01-25

著者

• Nakata Michinori

  Astronomical Institute Faculty Of Science Tohoku University

関連論文

• The Characteristic of the Large-amplitude Pulsation in a Model Yellow Supergiant Star
• Observational Constraint to the Minimum Flux Corona Model

スポンサーリンク