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Inverse problem of solar oscillations

  • Takashi Sekii
  • Hiromoto Shibahashi
The Sun
Part of the Lecture Notes in Physics book series (LNP, volume 274)

Abstract

We present some preliminary results of numerical simulation to infer the sound velocity distribution in the solar interior from the oscillation data of the Sun as the inverse problem. We analyze the acoustic potential itself by taking account of some factors other than the sound velocity, and we can infer fairly well the sound velocity distribution in the deep interior of the Sun.

Keywords

Inverse Problem Sound Velocity Solar Model Deep Interior Solar Interior 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Brodsky, M. A. and Vorontsov, S. V. 1986, in Advances in Helio-and Asteroseismology, IAU Symp. No.123, ed. J. Christensen-Dalsgaard (Reidel, Dordrecht), in press.Google Scholar
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  6. Shibahashi, H., Noels, A., and Gabriel, M. 1983, Astron. Astrophys., 123, 283.Google Scholar

Copyright information

© Springer-Verlag 1987

Authors and Affiliations

  • Takashi Sekii
    • 1
  • Hiromoto Shibahashi
    • 1
  1. 1.Department of AstronomyUniversity of TokyoTokyoJapan

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