Abstract
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.
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References
Abraham, Z. and Iben, I., Jr. Astrophys.J., 1971, 170, 157.
Brodsky, M. A. and Vorontsov, S. V., these proceedings.
Christensen-Dalsgaard, J. Mon.Not.Roy.Astron.Soc., 1985.
Libbrecht, K. G. and Zirin, H. Submitted to Astrophys.J.,1985.
Pidatella, R. M. and Stix, M. Astron.Astrophys., 1986, 157, 338.
Schmitt, J. H. M. M. and Rosner, R. Astrophys.J., 1983, 265, 901.
Spiegel, E. A. and Weiss, N. O. Nature, 1980, 287, 616.
Spruit, H. G. Solar Phys., 1974, 34, 277.
Vorontsov, S. V. Submitted to Proc. IAU Colloq. 90 ‘Upper main Sequence Stars with Anomalous Abundances’, Crimea, May 1985.
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© 1988 International Astronomical Union
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Vorontsov, S.V. (1988). A Search of the Effects of Magnetic Field in the Solar Five-Minute Oscillations. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_34
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DOI: https://doi.org/10.1007/978-94-009-4009-3_34
Publisher Name: Springer, Dordrecht
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