Effects of core mixing on solar oscillation frequencies
Conference
·
OSTI ID:6658441
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.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- DOE Contract Number:
- W-7405-ENG-36
- OSTI ID:
- 6658441
- Report Number(s):
- LA-UR-84-2448; CONF-840779-1; ON: DE84015540
- Resource Relation:
- Conference: 25. Liege international astrophysical colloquium, Leige, Belgium, 10 Jul 1984; Other Information: Portions are illegible in microfiche products
- Country of Publication:
- United States
- Language:
- English
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