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The Transfer of Large-scale Magnetic Field by Radial Inhomogeneity of the Material Density in the Rotating Convection Zone
Published online by Cambridge University Press: 12 April 2016
Abstract
The influence of rotation on the transfer of the mean magnetic field of the Sun, caused by the radial inhomogeneity of the solar turbulent plasma density, is investigated. It turns out that the transfer directions of the poloidal and toroidal magnetic fields do not coincide.
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- Part III Solar magnetism and large-scale flows
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- Copyright © Springer-Verlag 1991
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