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Last phases of development of active regions
Published online by Cambridge University Press: 14 August 2015
Abstract
A close relation of filament feet to the supergranular structure has been found. Green corona brightness, 1420 MHz flux, and the location of quiescent filaments depend upon the distribution of the photospheric magnetic fields. The development of polar maxima of the green corona and their relation to the following polarity have been studied.
- Type
- Part I: General Development of an Active Region
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- Copyright © Reidel 1968
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