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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

  • Lucio Paternó
Part II Physical Processes in Modelling the Sun
Part of the Lecture Notes in Physics book series (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.

Keywords

Convection Zone Solar Convection Zone Solar Standard Model Radial Order Adiabatic Oscillation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag 1990

Authors and Affiliations

  • Lucio Paternó
    • 1
    • 2
  1. 1.Istituto di AstronomiaUniversitá di CataniaItaly
  2. 2.CNR — Gruppo Nazionale di AstronomiaUdR di CataniaItaly

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