Dynamic dissipation of toroidal fields

Details Dynamic dissipation of toroidal fields Dynamic dissipation of toroidal fields

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maggi........8v&link_type=abstract

Magnitnaia Gidrodinamika (ISSN 0025-0015), Oct.-Dec. 1987, p. 8-14. In Russian.

Astronomy and Astrophysics

Astrophysics

Dynamo Theory, Energy Dissipation, Magnetic Field Configurations, Magnetoplasmadynamics, Rotating Plasmas, Toroidal Plasmas, Astrophysics, Electrodynamics, Magnetohydrodynamic Stability, Solar Interior

Scientific paper

A study is made of the nonequilibrium toroidal fields in the solar convection zone. These fields give rise to flow (which effectively mixes the the interior of the sun) and current layers, which are responsible for efficient field dissipation. It is shown that dissipation is no less efficient in a stratified medium in a gravitational field. The lifetime of toroidal fields in the solar convection zone is estimated.

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