Turbulent transfer of the large-scale magnetic field in the rotating convective zone of the sun

Details Turbulent transfer of the large-scale magnetic field in the rotating convective zone of the sun Turbulent transfer of the large-scale magnetic field in the rotating convective zone of the sun

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..842k&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 69, no. 4, p. 842-849.

Astronomy and Astrophysics

Astronomy

1

Magnetic Field Configurations, Poloidal Flux, Solar Convection (Astronomy), Solar Magnetic Field, Turbulent Diffusion, Magnetohydrodynamic Turbulence, Solar Cycles

Scientific paper

Consideration is given to the problem of the turbulent transfer of the large-scale magnetic field in a density-stratified convective zone, with the turbulence anisotropy excited by the sun's rotation taken into account. The anisotropy parameter (the Coriolis number - reciprocal of the Rossby number) and the transfer velocity components for the Spruit convective zone model are calculated. The transfer directions of the poloidal and toroidal components of the mean magnetic field do not coincide. The possible role of the turbulent transfer effects in the observed redistribution of magnetic fields over a solar cycle is discussed.

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