Physics – Atomic Physics
Scientific paper
Feb 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994an....315..157k&link_type=abstract
Astronomische Nachrichten (ISSN 0004-6337), vol. 315, no. 2, p. 157-170
Physics
Atomic Physics
136
Conductive Heat Transfer, Eddy Viscosity, Magnetic Diffusion, Magnetohydrodynamic Turbulence, Stellar Magnetic Fields, Stellar Rotation, Turbulent Diffusion, Anisotropy, Dynamo Theory, Quenching (Atomic Physics), Solar Convection (Astronomy), Stellar Models
Scientific paper
The old problem of turbulent diffusion is addressed to define the influence of rotation and magnetic field -- the usual ingredients of astrophysical bodies -- on the effective transport coefficients. Either rotation and magnetism produce the anisotropy and quenching. The tensorial structures of the diffusivities and their dependences on the angular velocity and the field strength are explicitly defined. An example of application of the theory to the global stellar circulation model is given and the implications for cosmic dynamos are briefly discussed.
Kitchatinov Leonid L.
Pipin Valery V.
Ruediger Guenther
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