Quasi-potential magnetic fields in stellar atmospheres. I - Static model of magnetic granulation

Details Quasi-potential magnetic fields in stellar atmospheres. I - Static model of magnetic granulation Quasi-potential magnetic fields in stellar atmospheres. I - Static model of magnetic granulation

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...298..235o&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 298, Nov. 1, 1985, p. 235-239.

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Magnetic Stars, Stellar Atmospheres, Stellar Magnetic Fields, Computational Astrophysics, Gravitational Fields, Magnetohydrodynamics, Quantum Mechanics

Scientific paper

Three-dimensional quasi-potential magnetic fields in stellar atmospheres are studied. Adopting the Clebsch (1859) representation for magnetic field and using the eigenvalue approach, a class of magnetic configurations capable of describing multilevel magnetic granulation is found. An example of a magnetic atmosphere with granulation is constructed in the form of an exact analytic solution of the basic equations. The corresponding quasi-potential magnetic field, in contrast to potential or force-free fields, is continuous everywhere and simultaneously has finite magnetic energy.

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