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A search of the effects of magnetic field in the solar five-minute oscillations
Published online by Cambridge University Press: 03 August 2017
Abstract
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An overshoot region near the base of the solar convection zone may be the region where intense magnetic fields are stored during the solar cycle (Spiegel and Weiss, 1980; Schmitt and Rosner, 1983; Pidatella and Stix, 1986). In this report we study the possible influence of such a field on the frequencies of the solar five-minute oscillations.
- Type
- Chapter 2: Theory of Solar Oscillations
- Information
- Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 151 - 154
- Copyright
- Copyright © Reidel 1988
References
Vorontsov, S.V.
Submitted to Proc. IAU Colloq. 90
‘Upper Main Sequence Stars with Anomalous Abundances’, Crimea, May
1985.CrossRefGoogle Scholar
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