Effects of core mixing on solar oscillation frequencies

Details Effects of core mixing on solar oscillation frequencies Effects of core mixing on solar oscillation frequencies

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984trss.conf..259c&link_type=abstract

Theoretical problems in stellar stability and oscillations, p. 259 - 263

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4

Diffusion, Electrostatics, Luminosity, Solar Oscillations, Turbulent Mixing, Concentration (Composition), Prediction Analysis Techniques, Reynolds Number, Temperature Effects

Scientific paper

This paper discusses predicted p- and g-mode periods for two solar models provided by Schatzman and Maeder (1981). One model has no mixing while the other has turbulent diffusion mixing (allowed for by a Reynolds number of 100). The resulting g-mode period spacings allow a very close look at the central solar structure which, like the p-mode period splittings, indicate little or no mixing over the lifetime of the Sun.

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