A solar model with a rotating magnetized core

Details A solar model with a rotating magnetized core A solar model with a rotating magnetized core

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apl....17..157s&link_type=abstract

Astrophysical Letters, vol. 17, no. 4, 1976, p. 157-161.

Physics

1

Solar Magnetic Field, Solar Physics, Solar Rotation, Stellar Models, Kelvin-Helmholtz Instability, Magnetohydrodynamic Stability, Neutrinos, Particle Flux Density

Scientific paper

Models of the sun are constructed which possess cores in which rotational and magnetic-field energy are in equipartition. These cores are formally spherically symmetric and appear to be stable toward turbulence and, except for the most extreme case, toward bar-mode instability. Such models are capable of producing a neutrino flux as low as 0.64 SNU.

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