Effects of core mixing on solar oscillation frequencies
Description:
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.
Date:
July 27, 1984
Creator:
Cox, A. N. & Kidman, R. B.
Item Type:
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