Magnetic fields in media with differential rotation. I

Details Magnetic fields in media with differential rotation. I Magnetic fields in media with differential rotation. I

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..297b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Mar.-Apr. 1985, p. 297-301. In Russian.

Statistics

Computation

Computational Astrophysics, Magnetic Field Configurations, Planetary Rotation, Rotating Matter, Stellar Rotation, Angular Velocity, Diffusion Coefficient, Planetary Magnetic Fields, Radii, Saturn (Planet), Stellar Magnetic Fields

Scientific paper

The paper derives equations describing the behavior of arbitrary nonaxisymmetric magnetic fields in a differentially rotating medium with a magnetic diffusion coefficient that depends only on radius. These equations are used to obtain results that can explain the absence of magnetic fields in certain rapidly rotating stars. Particular attention is given to the magnetic field of Saturn.

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