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Opposite Polarities in the Development of Some Regularities in the Distribution of Large-Scale Magnetic Fields

Published online by Cambridge University Press:  14 August 2015

P. Ambrož ,
V. Bumba ,
R. Howard  and
J. Sýkora
P. Ambrož
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
V. Bumba
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
R. Howard
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
J. Sýkora
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia

Abstract

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When viewed separately in the two polarities, the large-scale pattern of magnetic fields on the Sun gives an appearance reminiscent of a very large cellular structure. These structures and their relation to ‘active longitudes’ are discussed.

Type
Part VII: The Polar Fields of the Sun and the Magnetic Activity Cycle
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 696 - 709
Copyright
Copyright © Reidel 1971 

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