Last phases of development of active regions
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Published:1968
Issue:
Volume:35
Page:64-67
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ISSN:0074-1809
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Container-title:Symposium - International Astronomical Union
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language:en
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Short-container-title:Symp. - Int. Astron. Union
Author:
Bumba V.,Kleczek J.,Olmr J.,Růžičková-Topolová B.,Sýkora J.
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.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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