Physics
Scientific paper
May 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8916713g&link_type=abstract
Presented at the Seismology of the Sun and Sun-Like Stars, Puerto de la Cruz, Spain, 26 Sep. 1988
Physics
Asymptotic Methods, Gravitational Fields, Periodic Functions, Solar Gravitation, Asymptotic Properties, Sun
Scientific paper
The asymptotic properties of the low-degree solar gravity modes classified by Hill and Gu are studied in the framework of first- and second-order asymptotic theory predictions. The results of this analysis demonstrate the necessity of retaining the second-order term in asymptotic theory to describe the eigenfrequency spectrum. In this theory, there are two first-order parameters, Tomicron and delta, and two second-order parameters, V1 and V2. Values of the parameters obtained in this analysis are: Tomicron = 36.31 + or - 0.12 min, delta = minus 0.43 + or - 0.13, V1 = 0.35, and V2 = 4.76. There remain differences of approx. 0.3 micro-Hz between the asymptotic theory eigenfrequencies and observed eigenfrequencies which are quasi-periodic functions of the radial order n for a given value of the degree ell.
Gu Ye-Ming
Hill Henry A.
Rosenwald Ross D.
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