Magnetic Diffusion in Stratified Atmospheres

Details Magnetic Diffusion in Stratified Atmospheres Magnetic Diffusion in Stratified Atmospheres

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spd....28.0251d&link_type=abstract

American Astronomical Society, SPD meeting #28, #02.51; Bulletin of the American Astronomical Society, Vol. 29, p.902

Astronomy and Astrophysics

Astronomy

Scientific paper

The predictions from of Mean Field Electrodynamics have been questioned because of the strong feedback of small scale magnetic structures on the velocity fields. In 2-D, this nonlinear feedback results in a lengthening of the turbulent decay time. In 3-D alpha -quenching is predicted. Previous studies assumed a homogeneous fluid. We will present recent results from 2-D compressible MHD decay simulations in a highly stratified atmosphere that more closely resembles to solar convection zone.

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