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Second-order asymptotic theory of solar acoustic oscillations

  • S. V. Vorontsov
Part II Physical Processes in Modelling the Sun
Part of the Lecture Notes in Physics book series (LNP, volume 367)

Abstract

The second-order asymptotic theory is developed for low- and intermediate-degree acoustic oscillations of the Sun and Sun-like stars, in a form convenient to use for helioseismic inversions.

Keywords

Acoustic Oscillation Solar Model Solar Interior Nonlinear Inversion Solar Core 
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. Kosovichev, A.G. 1988, in Seismology of the Sun and Sun-like Stars, ed. E. Rolfe, ESA SP-286 (ESA Publication Division, Noordwijk), p.533.Google Scholar
  2. Vorontsov, S.V. 1988, in Seismology of the Sun and Sun-like Stars, ed. E. Rolfe, ESA SP-286 (ESA Publication Division, Noordwijk), p.475.Google Scholar
  3. Vorontsov, S.V., and Zharkov, V.N. 1989, Soviet Sci. Rev. E, Astrophys. Space Phys. Rev., 7, 1.Google Scholar
  4. Woodhouse, J.H. 1978, Geophys. J. Roy. Astron. Soc., 54, 263.Google Scholar

Copyright information

© Springer-Verlag 1990

Authors and Affiliations

  • S. V. Vorontsov
    • 1
  1. 1.Institute of Physics of the EarthMoscowUSSR

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