Compressible magnetic convection - Formulation and two-dimensional models

Details Compressible magnetic convection - Formulation and two-dimensional models Compressible magnetic convection - Formulation and two-dimensional models

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...383..860f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 383, Dec. 20, 1991, p. 860-881.

Computer Science

Sound

19

Convection, Magnetohydrodynamics, Solar Granulation, Solar Interior, Solar Magnetic Field, Dynamo Theory, Magnetoacoustics, Magnetohydrodynamic Waves, Sound Waves, Two Dimensional Models

Scientific paper

Details on a formulation and numerical solution of the equations of time-dependent magnetized convection are presented. Results on the transition between weak and strong magnetic fields where the highly nonlinear behavior commences are discussed, and the sensitivity of these results to the value of the magnetic resistivity, which can significantly influence the details of the interactions, is indicated. Consideration is given to the consequences of the findings for modeling stellar and solar magnetic fields.

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