Abstract
By using the quantization rule based on the WKB asymptotic method, we present an integral equation to infer the form of the acoustic potential of a fixed ℓ as a function of the acoustic length. Since we analyze the acoustic potential itself by taking account of some factors other than the sound velocity and we can analyze the radial modes by this scheme as well as nonradial modes, this method improves the accuracy and effectiveness of the inverse problem to infer the internal structure of the Sun, in particular, the deep interior of the Sun.
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References
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© 1988 International Astronomical Union
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Shibahashi, H. (1988). Inverse Problem: Acoustic Potential vs Acoustic Length. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_30
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DOI: https://doi.org/10.1007/978-94-009-4009-3_30
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2615-5
Online ISBN: 978-94-009-4009-3
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