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Turbulent Transport of Magnetic Fields and the Solar Dynamo

Published online by Cambridge University Press:  19 July 2016

L.L. Kichatinov
L.L. Kichatinov*
Affiliation:
Astrophysikalisches Institut Potsdam An der Sternwarte 16, D-O-1590 Potsdam, Germany

Abstract

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The effect of anisotropic transport of the mean magnetic field by turbulence in a stratified rotating fluid is briefly discussed to find its qualitative correspondence to the observed field redistribution over a solar cycle. A kinematic model of a dynamo in a spherical shell is developed with the transport effect included to assess its importance in a more consistent way. The anisotropic transport brings the simulated field behavior closer to that observed on the Sun.

Type
1. The Solar Dynamo
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 13 - 17
Copyright
Copyright © Kluwer 1993 

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