Solar models with differential rotation and toroidal magnetic fields

Details Solar models with differential rotation and toroidal magnetic fields Solar models with differential rotation and toroidal magnetic fields

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...290..337t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 290, March 1, 1985, p. 337-343. Research supported by the U.S. Department o

Astronomy and Astrophysics

Astrophysics

1

Magnetic Field Configurations, Solar Magnetic Field, Solar Neutrinos, Solar Oblateness, Solar Rotation, Differential Equations, Hydrodynamics, Integral Equations, Legendre Functions

Scientific paper

Solar models which could possibly solve the solar neutrino problem without incorporating neutrino oscillations are discussed. In particular it is found that it is possible to have solar models with rapid differential rotation and low surface oblateness, if one allows for the presence of strong toroidal magnetic fields with the proper configuration.

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