Magnetic star models - Toroidal fields and circulation

Details Magnetic star models - Toroidal fields and circulation Magnetic star models - Toroidal fields and circulation

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.178...51m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 178, Jan. 1977, p. 51-59.

Astronomy and Astrophysics

Astronomy

20

Atmospheric Circulation, Magnetic Field Configurations, Magnetic Stars, Stellar Atmospheres, Stellar Models, Angular Velocity, Perturbation Theory, Steady State, Stellar Magnetic Fields, Stellar Rotation, Toroidal Shells

Scientific paper

Models of uniformly rotating magnetic stars containing mixed poloidal-toroidal fields of even parity and the associated thermally-driven circulation are constructed by a first-order perturbation method. At given angular velocity and large-scale surface field, increasing the toroidal field decreases the interior poloidal field. The range of internal fluxes available to models is somewhat increased by the inclusion of a toroidal field, but there remain values of the angular velocity and internal flux for which no solutions can be found.

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