The adiabatic stability of stars containing magnetic fields. V Effect of ohmic diffusion on stable fields

Details The adiabatic stability of stars containing magnetic fields. V Effect of ohmic diffusion on stable fields The adiabatic stability of stars containing magnetic fields. V Effect of ohmic diffusion on stable fields

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.198..811t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 198, Mar. 1982, p. 811-815.

Astronomy and Astrophysics

Astronomy

12

Magnetic Flux, Main Sequence Stars, Ohmic Dissipation, Stellar Magnetic Fields, Adiabatic Conditions, Magnetic Diffusion, Stellar Evolution, Stellar Interiors, Stellar Models, Stellar Structure, Toroids

Scientific paper

In previous papers it has been shown that dynamically stable strong magnetic fields in stellar interiors must have mixed poloidal/toroidal character. It is now shown that such stable fields probably diffuse into unstable configurations in a time which is less than a stellar main-sequence lifetime. This indicates that it is less likely than was previously thought that strong internal fields will survive the main-sequence lifetime of a star.

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