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The Coronal Responses to the Large-Scale and Long-Term Phenomena of the Lower Layers of the Sun

Published online by Cambridge University Press:  14 August 2015

J. Sýkora
J. Sýkora*
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, Skalnaté Pleso, 059 60 Tatranská Lomnica, Czechoslovakia

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Based on the assumption, generally accepted over the past decade, that all the forms of solar and interplanetary activity are responses to the magnetic fields generated initially in the subphotosphere, some characteristics of the large-scale and long-term behaviour of the solar corona during the last three solar cycles are presented.

Type
Part II. Coronal and Interplanetary Responses to Long Time Scale Phenomena
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 87 - 104
Copyright
Copyright © Reidel 1980 

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