The stability of solar gravity-mode oscillations and the structure of the sun

Details The stability of solar gravity-mode oscillations and the structure of the sun The stability of solar gravity-mode oscillations and the structure of the sun

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..679k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Sept. 1984, p. 679-684) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Sept.-O

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Solar Oscillations, Stellar Models, Stellar Structure, Chemical Composition, Computational Astrophysics, Heavy Elements, Solar Interior, Solar Neutrinos, Turbulent Diffusion

Scientific paper

The g-mode oscillations stability for the interior of solar models with low heavy-element abundances and models with turbulent diffusion mixing inside is investigated by a quasi-adiabatic approximation. The models with low Z are found to be most unstable. It is pointed out that only the models with low Z are in agreement with the solar neutrino experiment and the observed solar gravity mode oscillations.

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