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Resonant Coupling Between Solar Gravity Modes

Invited Review

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Problems of Solar and Stellar Oscillations

Abstract

It is shown that in consequence of the parametric resonance, g modes of low spherical harmonic degree l are strongly coupled to the modes of high degree. The coupling limits the growth of lowl modes to very small amplitudes. For gl, l = 1 mode, the final amplitude of the radial velocity is of the order of 10 cm s-1. A mixing of solar core as a result of a finite-amplitude development of linear instability of this mode is thus highly unlikely.

Proceedings of the 66th IAU Colloqium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.

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Author information

Authors and Affiliations

  1. N. Copernicus Astronomical Center, 00-716, Warsaw, Poland

    W. Dziembowski

Authors
  1. W. Dziembowski
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Editor information

Editors and Affiliations

  1. Institute of Astronomy, Cambridge, USA

    D. O. Gough

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© 1983 D. Reidel Publishing Co, Dordrecht, Holland, and Boston, U.S.A.

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Dziembowski, W. (1983). Resonant Coupling Between Solar Gravity Modes. In: Gough, D.O. (eds) Problems of Solar and Stellar Oscillations. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7088-5_29

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  • DOI: https://doi.org/10.1007/978-94-009-7088-5_29

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7090-8

  • Online ISBN: 978-94-009-7088-5

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