対流崩壊による太陽微細磁束管の形成(対流(3),一般講演)

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概要

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• The solar surface, photosphere, is covered with magnetic flux tubes with kilo gauss field strength and spatial scale of 〜200km. It has been believed that those flux tubes area formed through convective instability, however the hypotheses has lacked the observational support so far. The Solar Optical Telescope of Hinode revealed the formation of those flux tubes for the first time. The observation is well explained with the theoretical model predicted thirty years ago.

• 日本流体力学会の論文
• 2008-09-04

著者

• 永田 伸一

  京大理天文台

関連論文

• 対流崩壊による太陽微細磁束管の形成(対流(3),一般講演)

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