Effect of solar rotation on turbulent transfer of the large-scale magnetic field in the convective zone

Details Effect of solar rotation on turbulent transfer of the large-scale magnetic field in the convective zone Effect of solar rotation on turbulent transfer of the large-scale magnetic field in the convective zone

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...30k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Nov.-Dec. 1991, p. 30-39. In Ukrainian.

Computer Science

Convective Flow, Magnetohydrodynamic Turbulence, Solar Magnetic Field, Solar Rotation, Equations Of Motion, Solar Cycles, Stellar Envelopes

Scientific paper

The turbulent transfer of the large-scale magnetic field is investigated in the density-stratified convective zone with due regard for turbulence anisotropy excited by solar rotation. It is found that the transfer directions of poloidal and toroidal components of the magnetic field do not coincide in the rotating convective envelope. The values of different transfer velocity components of the magnetic fields for the Spruit convective zone model are calculated. The possible role of the transport effects in the large-scale field dynamics over a solar cycle is discussed.

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