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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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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