The instability of strong magnetic fields in stellar interiors

Details The instability of strong magnetic fields in stellar interiors The instability of strong magnetic fields in stellar interiors

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..31..261p&link_type=abstract

Astrophysics and Space Science, vol. 31, Nov. 1974, p. 261-266.

Astronomy and Astrophysics

Astrophysics

31

Buoyancy, Magnetic Flux, Magnetic Variations, Neutrinos, Solar Magnetic Field, Stellar Interiors, Astronomical Models, Gas Pressure, Magnetic Effects, Paleomagnetism, Solar Corpuscular Radiation, Solar Interior

Scientific paper

There has been discussion of the possibility of resolving the solar neutrino dilemma with a sufficiently strong magnetic field (500 MG) in the solar interior to relieve the gas pressure by some 10% or more. The time in which magnetic buoyancy will bring a strong field to the surface is examined and is found to be less than 100 m.y. No possibility is seen for retaining a suitably strong magnetic field in the solar interior.

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