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Turbulent Transport of Magnetic Fields and the Solar Dynamo
Published online by Cambridge University Press: 19 July 2016
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
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- Copyright
- Copyright © Kluwer 1993
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