Constraints of observations of solar oscillations on solar models with mixing by turbulent diffusion
- 1 January 1985
- proceedings article
- Published by AIP Publishing in AIP Conference Proceedings
- Vol. 126 (1) , 93-99
- https://doi.org/10.1063/1.35173
Abstract
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 3 7Cl experiment are in conflict with published solar oscillation data.Keywords
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