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Generation of Strong Toroidal Magnetic Field Near the Bottom of the Solar Convective Zone
Published online by Cambridge University Press: 12 April 2016
Abstract
The generation mechanism of the toroidal magnetic field by the angular velocity radial gradient acting on the relict poloidal magnetic field on the boundary between the con-vective and radiative zones is proposed. The magnetic induction magnitude of the toroidal field reaches about 2×10σ G, the limiting effect of the magnetic buoyancy being taking into account. This value conforms to the estimation of toroidal field obtained from helioseismological data.
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- I. Setting the stage: Sun, Stars Galaxies and the Universe
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- Copyright © Astronomical Society of the Pacific 1993