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Advances in Solar Physics pp 29–40Cite as

The structure of the solar core

  • Part I Solar Internal Structure
  • Conference paper
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Part of the book series: Lecture Notes in Physics ((LNP,volume 432))

Abstract

The efforts to resolve the solar neutrino problem resulted in a considerable progress in reliability and accuracy in modelling the Sun's interior. Implications from helioseismic sounding supports the standard picture of the solar evolution. A comparison of neutrino fluxes measured in various experiments seems to rule out a non-standard solar core as the solution of the neutrino problem.

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Author information

Authors and Affiliations

  1. Astronomy Unit, Queen Mary and Westfield College, University of London, ul.Bartycka 18, 00-716, Warsaw, Poland

    W. A. Dziembowski

  2. Copernicus Astronomical Center, ul.Bartycka 18, 00-716, Warsaw, Poland

    W. A. Dziembowski

Authors
  1. W. A. Dziembowski
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Editor information

G. Belvedere M. Rodonò G. M. Simnett

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© 1994 Springer-Verlag

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Dziembowski, W.A. (1994). The structure of the solar core. In: Belvedere, G., Rodonò, M., Simnett, G.M. (eds) Advances in Solar Physics. Lecture Notes in Physics, vol 432. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-58041-7_198

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  • DOI: https://doi.org/10.1007/3-540-58041-7_198

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-58041-6

  • Online ISBN: 978-3-540-48420-2

  • eBook Packages: Springer Book Archive

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