Constraints of observations of solar oscillations on solar models with mixing by turbulent diffusion

Details Constraints of observations of solar oscillations on solar models with mixing by turbulent diffusion Constraints of observations of solar oscillations on solar models with mixing by turbulent diffusion

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aipc..126...93c&link_type=abstract

IN: Solar neutrinos and neutrino astronomy; Proceedings of the Conference, Lead, SD, August 23-25, 1984 (A86-37626 17-93). New Y

Astronomy and Astrophysics

Astrophysics

6

Astrophysics, Solar Oscillations, Stellar Models, Turbulent Diffusion, Frequency Response, Mixing, Reynolds Number, Solar Neutrinos

Scientific paper

The pulsational behavior of solar models with mixing produced by turbulent diffusion has been investigated, for both p (pressure) modes and g (gravity) modes. It is found that while a small amount of mixing may be allowed by the observed data on solar oscillations, values of the pseudo-Reynolds number large enough to reduce the predicted neutrino counting rate to the level seen by the 37Cl experiment are in conflict with published solar oscillation data.

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