Computer Science – Numerical Analysis
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376l..21c&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 376, July 20, 1991, p. L21-L24. NASA-supported research.
Computer Science
Numerical Analysis
163
Magnetic Diffusion, Magnetohydrodynamics, Stellar Magnetic Fields, Transport Properties, Turbulent Diffusion, Equipartition Theorem, Numerical Analysis, Two Dimensional Models
Scientific paper
Two-dimensional numerical simulations with high spatial resolution are used to study the effects of a large-scale magnetic field on its turbulent transport. It is commonly believed that the nonlinear back-reaction of the magnetic field on the turbulence becomes important when the field strength is close to equipartition. However, turbulent diffusion is effectively reduced even when the large-scale field is much weaker than equipartition.
Cattaneo Fausto
Vainshtein Samuel I.
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