Influence of the Upper Layers of the Sun on the p-Mode Frequencies

Christensen-Dalsgaard, J.; Pérez Hernández, F.
Bibliographical reference

Challenges to Theories of the Structure of Moderate-Mass Stars, Proceedings of a Conference held at the Institute for Theoretical Physics, University of California, Stnta Barbara, CA, USA, 19-22 June 1990. Edited by D. Gough and J. Toomre. Springer-Verlag Berlin Heidelberg New York. Also Lecture Notes in Physics, volume 388, 1991, p.43

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1991
Number of authors
2
IAC number of authors
0
Citations
30
Refereed citations
27
Description
We consider the effect of uncertainties in solar models on the p-mode frequencies of moderate degree (40 l 100). This is done by means of an asymptotic relation that provides a simple way of estimating differences in p-mode frequencies of two solar models. Also, we have investigated the possibility for separating different contributions to the difference between the models, on the basis of the frequencies of the modes. Analysis of observed frequencies suggests that the solar envelope helium abundance Y s is close to 0.25; however, this result may be sensitive to other uncertainties in the solar models.
Type