Hostname: page-component-cc8bf7c57-pd9xq Total loading time: 0 Render date: 2024-12-12T07:59:17.012Z Has data issue: false hasContentIssue false

A search of the effects of magnetic field in the solar five-minute oscillations

Published online by Cambridge University Press:  03 August 2017

S. V. Vorontsov*
Affiliation:
Institute of Physics of the Earth, B. Gruzinskaya 10, 123810 Moscow, USSR

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Reidel 1988 

References

Abraham, Z. and Iben, I. Jr. Astrophys. J., 1971, 170, 157.Google Scholar
Brodsky, M.A. and Vorontsov, S.V., these proceedings. Google Scholar
Christensen-Dalsgaard, J. Mon. Not. Roy. Astron. Soc., 1932, 199, 735.Google Scholar
Libbrecht, K.G. and Zirin, H. Submitted to Astrophys. J., 1985.Google Scholar
Pidatella, R.M. and Stix, M. Astron. Astrophys., 1986, 157, 338.Google Scholar
Schmitt, J.H.M.M. and Rosner, R. Astrophys. J., 1983, 265, 901.Google Scholar
Spiegel, E.A. and Weiss, N.O. Nature, 1980, 287, 616.Google Scholar
Spruit, H.G. Solar Phys., 1974, 34, 277.Google Scholar
Vorontsov, S.V. Submitted to Proc. IAU Colloq. 90 ‘Upper Main Sequence Stars with Anomalous Abundances’, Crimea, May 1985.CrossRefGoogle Scholar