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III. The Solar Dynamo

Published online by Cambridge University Press:  25 April 2016

M. Stix

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Traditionally the theory of the solar dynamo has been divided into two parts. The first, more difficult part, is the derivation of equations governing the mean magnetic field; the second, easier, is the solution of this equation, and the interpretation of the result in terms of observed solar magnetism. This report follows the traditional division.

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 20 , Issue 1 , 1988 , pp. 94 - 97
Copyright
Copyright © Kluwer 1988 

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