Turbulence in a rotating magnetized fluid

Details Turbulence in a rotating magnetized fluid Turbulence in a rotating magnetized fluid

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994an....315..151p&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 315, no. 2, p. 151-156

Astronomy and Astrophysics

Astronomy

Magnetohydrodynamic Flow, Magnetohydrodynamic Turbulence, Rotating Fluids, Toroidal Plasmas, Turbulence Models, Turbulent Flow, Convection Cells, Coriolis Effect, Solar Convection (Astronomy), Solar Magnetic Field, Stokes Flow

Scientific paper

In a quasilinear approximation, for a special model of initial turbulence the combined effect of the rotation and the large-scale toriodal magnetic field was calculated. For large values of parameters of magnetic field strength and the rotation rate of the medium. With increasing magnetic field strength and rotation rate, the inhomogeneity scale of turbulence increases in the direction of both the magnetic field and the angular velocity vector.

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