Abstract
An asymptotic analysis of stellar p modes in the short-wavelength limit is summarized. The formula can be used as a means of estimating the sound speed in the solar interior from a knowledge of identified eigenfrequencies. The accuracy of the procedure is discussed and it is shown how the results can be used to measure properties such as the location of the base of the convection zone.
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© 1986 D. Reidel Publishing Company, Dordrecht, Holland
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Gough, D.O. (1986). Asymptotic Sound-Speed Inversions. In: Gough, D.O. (eds) Seismology of the Sun and the Distant Stars. NATO ASI Series, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4608-8_14
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DOI: https://doi.org/10.1007/978-94-009-4608-8_14
Publisher Name: Springer, Dordrecht
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