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A Numerical Study of the Solar Cycle

Published online by Cambridge University Press:  14 August 2015

Y. Nakagawa*
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research*, Boulder, Colo., U.S.A.

Abstract

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Models relevant to numerical studies of the solar cycle are reviewed briefly with discussions of pertinent physical mechanisms. It is suggested that the observed surface activities are secondary in nature and an example of possible non-axisymmetric steady state solutions is given, together with the results of preliminary numerical computations.

Type
Part VII: The Polar Fields of the Sun and the Magnetic Activity Cycle
Copyright
Copyright © Reidel 1971 

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