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Origin of the Sun's Differential Rotation

Published online by Cambridge University Press:  08 February 2017

L.L. Kichatinov
L.L. Kichatinov*
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (SibIZMIR) 664697 Irkutsk, P.O. Box 4 USSR

Abstract

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The present status of the Sun's differential rotation theories is reviewed. Attention is mainly focused on mechanisms for differential rotation based on the anisotropic viscosity concept and their modern developments within the framework of the mean-field hydrodynamics. The models with latitude-dependent heat transport and non-axisymmetric numerical simulations are briefly discussed.

Type
V. Large-scale Structure and Dynamics
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 297 - 307
Copyright
Copyright © Kluwer 1990 

References

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