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Structure of the solar Core inferred from inversion of frequencies of low-degree p-modes

  • Part V Inverse Problems of Solar Oscillations
  • Conference paper
  • First Online:
Progress of Seismology of the Sun and Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 367))

Abstract

Results of estimations of density and a parameter of convective stability in the central regions of the Sun from observed frequencies of 5-min modes are presented.

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Author information

Authors and Affiliations

  1. Crimean Astrophysical Observatory, Nauchny, 334413, Crimea, USSR

    A. G. Kosovichev

Authors
  1. A. G. Kosovichev
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Editor information

Y. Osaki H. Shibahashi

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© 1990 Springer-Verlag

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Kosovichev, A.G. (1990). Structure of the solar Core inferred from inversion of frequencies of low-degree p-modes. In: Osaki, Y., Shibahashi, H. (eds) Progress of Seismology of the Sun and Stars. Lecture Notes in Physics, vol 367. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53091-6_94

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  • DOI: https://doi.org/10.1007/3-540-53091-6_94

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-53091-6

  • Online ISBN: 978-3-540-46645-1

  • eBook Packages: Springer Book Archive

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