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Effects of overshooting and magnetic field at the base of the solar convection zone on the 5-minute p-mode eigenfrequencies

  • Part II Physical Processes in Modelling the Sun
  • 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

The effect of an overshooting layer at the base of the solar convection zone, where a magnetic field can be intensified to largely exceed the equipartition value, on the p-mode eigen-frequencies is investigated and the results are compared with observations.

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Authors and Affiliations

  1. Istituto di Astronomia, Universitá di Catania, Italy

    Lucio Paternó

  2. CNR — Gruppo Nazionale di Astronomia, UdR di Catania, Italy

    Lucio Paternó

Authors
  1. Lucio Paternó
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Editor information

Y. Osaki H. Shibahashi

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© 1990 Springer-Verlag

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Paternó, L. (1990). Effects of overshooting and magnetic field at the base of the solar convection zone on the 5-minute p-mode eigenfrequencies. 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_62

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  • DOI: https://doi.org/10.1007/3-540-53091-6_62

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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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