The magnetic flux in the quiet sun network
作者： Barry J. Labonte , Robert Howard
DOI: 10.1007/BF00153420
关键词:
摘要: The Ca ii K line emission from the quiet Sun network does not vary with 11-year cycle (White and Livinston, 1981). We confirm this result direct magnetic measurements. This effect is simply explained by present empirical models of evolution surface fields.
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