The magnetic flux in the quiet sun network |
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| Authors: | Barry J Labonte Robert Howard |
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| Institution: | (1) Mount Wilson and Las Campanas Observatories of the Carnegie Institution of Washington, Washington, U.S.A. |
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| Abstract: | The Ca ii K line emission from the quiet Sun network does not vary with the 11-year cycle (White and Livinston, 1981). We confirm this result from direct magnetic measurements. This effect is not simply explained by present empirical models of the evolution of surface magnetic fields.Now at Institute for Astronomy, University of Hawaii, Honolulu, Hawaii 96822, U.S.A. |
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