Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..803k&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Sept. 1987, p. 803-810. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
2
Convective Heat Transfer, Magnetic Flux, Plasma Turbulence, Solar Magnetic Field, Buoyancy, Density Distribution, Flow Velocity, Plasma Density, Radial Distribution
Scientific paper
The transfer velocity of the horizontal large-scale magnetic field in the Sun due to the radial density gradient of the solar turbulent plasma is calculated in a nonlinear approach for three mixing length models of the convective zone. The value of the transfer velocity is changed from 104cm/s in the surface layers to 102cm/s near the deep layers of the convective zone bottom. Maximum values of the stationary magnetic field in the deep layers of the convective zone are estimated which is conserved under the joint action of the magnetic buoyancy and downward flux of the magnetic field due to the radial gradient of the matter density.
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