Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-30T00:40:16.726Z Has data issue: false hasContentIssue false
  • English
  • Français

The magnetic field inside the Sun

Published online by Cambridge University Press:  03 August 2017

W. Dziembowski  and
Philip R. Goode
W. Dziembowski
Affiliation:
N. Copernicus Center, Polish Academy of Sciences, Warsaw, Poland
Philip R. Goode
Affiliation:
Department of Physics, New Jersey Institute of Technology Newark, New Jersey, USA

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.

Duvall, Harvey and Pomerantz (1986) reported the existence of a ‘structural asymmetry’ inside the Sun. We show that this asymmetry is not a consequence of the Sun's rotation. We attribute the asymmetry, rather, to a toroidal magnetic field inside the Sun. Consistency requires a field of about one megagauss located in the lower part of the convection zone. Accounting for such a field would wreak havoc on our understanding of the solar dynamo and convection.

Type
Chapter 2: Theory of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 171 - 174
Copyright
Copyright © Reidel 1988 

References

Duvall, T.L. Jr., Dziembowski, W.A., Goode, P.R., Gough, D.O., Harvey, J.W. and Leibacher, J.W., Nature, 310, 22 (1984).CrossRefGoogle Scholar
Duvall, T.L. Jr., Harvey, J.W. and Pomerantz, M.A., Nature, 321, 500 (1986).CrossRefGoogle Scholar
Mestel, L. and Moss, D.L., Mon. Not. R. Astr. Soc. 178, 27 (1977).Google Scholar