The D(nl) values and the structure of the solar core

Details The D(nl) values and the structure of the solar core The D(nl) values and the structure of the solar core

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...226..278g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 226, no. 1, Dec. 1989, p. 278-283.

Astronomy and Astrophysics

Astrophysics

19

Solar Interior, Solar Oscillations, Stellar Cores, Stellar Structure, Asymptotic Methods, Gravitational Effects, Perturbation

Scientific paper

This paper presents calculations of the Cowling approximation D(nl) (where n and l are the order and the degree of the mode), computed from the Gough (1984, 1986) formula for nu(n,l). Also computed are values of D(nl) and Delta D(n). It is shown that, contrary to the results of Gough, the layers above the turning point of the (n - 1,l + 2) mode contribute significantly to Delta D(n). It is found that, when the perturbation of the gravitational potential are taken into account for evaluations of D(nl) and Delta D(n), all layers inside the solar sphere extending over 25 to 35 percent of the total radius contribute significantly to both of these quantities.

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