Physics
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..403h&link_type=abstract
In ESA, Seismology of the Sun and Sun-Like Stars p 403-406 (SEE N89-25819 19-92)
Physics
2
Asymptotic Properties, Eigenvalues, Solar Gravitation, Solar Oscillations, Fine Structure, Molecular Weight, Solar Interior
Scientific paper
The fine structure found by Gu, Hill, and Rosenwald (1988) between asymptotic theory eigenfrequencies and the observed eigenfrequencies reported by Hill and Gu is interpreted as the result of conditions not being met for the applicability of asymptotic theory at one or more radii in the solar interior. From an inversion of the observed fine structure, reasonably good agreement is obtained between observation and theory for either a localized perturbation in internal structure at r/R = 0.06 or at r/R = 0.23. The latter solution is, however, the better one. The amplitude of the perturbation in the mean molecular weight required to produce the fine structure is also inferred.
Gao Qiang
Hill Henry A.
Rosenwald Ross D.
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