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Five minute oscillations as a probe of the solar interior

  • 3. Solar Oscillations
  • Conference paper
  • First Online:
Nonradial and Nonlinear Stellar Pulsation

Part of the book series: Lecture Notes in Physics ((LNP,volume 125))

Abstract

The solar five minute oscillation has been shown to consist of a large number of nonradial acoustic modes. Observations of these modes provide a probe of the solar interior; specifically tests on models of the solar convection zone.

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References

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Author information

Authors and Affiliations

  1. Department of Astronomy, University of California at Los Angeles, USA

    S. H. Lubow, E. J. Rhodes Jr. & R. K. Ulrich

Authors
  1. S. H. Lubow
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  2. E. J. Rhodes Jr.
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  3. R. K. Ulrich
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Editor information

H. A. Hill W. A. Dziembowski

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© 1980 Springer-Verlag

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Lubow, S.H., Rhodes, E.J., Ulrich, R.K. (1980). Five minute oscillations as a probe of the solar interior. In: Hill, H.A., Dziembowski, W.A. (eds) Nonradial and Nonlinear Stellar Pulsation. Lecture Notes in Physics, vol 125. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-09994-8_28

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  • DOI: https://doi.org/10.1007/3-540-09994-8_28

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-09994-9

  • Online ISBN: 978-3-540-39297-2

  • eBook Packages: Springer Book Archive

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