Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-08T00:32:36.020Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Field in the Sun’s Interior from Oscillation Data

Published online by Cambridge University Press:  12 April 2016

W.A. Dziembowski  and
P.R. Goode
W.A. Dziembowski
Affiliation:
Copernicus Astronomical Center, Warszawa, Poland
P.R. Goode
Affiliation:
Department of Physics, N.J.I.T., Newark, NJ, 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.

Solar oscillations provide a probe of the internal magnetic field of the Sun if the field has sufficient intensity. Using the oscillation data of Libbrecht, we find evidence for a 2 ± 1 megagauss quadrupole toroidal field centered at 0.7 of the solar radius which is barely beneath the base of the convection zone. This field, by its location and symmetry, may be associated with the dynamo that drives the Sun’s 22-year activity cycle.

Type
Part 3: Helioseismology
Information
International Astronomical Union Colloquium , Volume 121: Inside the Sun , 1990 , pp. 341 - 348
Copyright
Copyright © Kluwer 1990

References

Backus, G. and Gilbert, F. 1970, Phil. Trans Roy. Soc. London A 266, 12.Google Scholar
Brodsky, M.A. and Vorontsov, S.V. 1988, Advances in Helio- and Asteroseismology, 137, Christensen-Dalsgaard, J. and Fransden, S. (Eds.), Reidel, Dordrecht, the Netherlands.Google Scholar
Brown, T.M., Christensen-Dalsgaard, J., Dziembowski, W.A., Goode, P.R., Gough, D.O., and Morrow, C.A. 1989, Ap.J., in press.Google Scholar
Brown, T.M. and Morrow, C.A. 1987, Ap. J. Lett. 314, L21.Google Scholar
Christensen-Dalsgaard, J., Duvall, T.J., Gough, D.O., Harvey, J.W. and Rhodes, E.J. 1985, Nature 315, 378.Google Scholar
Christensen-Dalsgaard, J. and Shou, J. 1988, Seismology of the Sun and Sun-like Stars, 149, Rolfe, E.J. (Ed.), ESA, Noordwijk, The Netherlands.Google Scholar
Duvall, T.J., Dziembowski, W.A., Goode, P.R., Gough, D.O., Harvey, J.W. and Leibacher, J.W. 1984, Nature 310, 22.Google Scholar
Duvall, T.J., Harvey, J.W. and Pomerantz, M.A. 1986, Nature 321, 500.Google Scholar
Dziembowski, W.A. and Goode, P.R. 1989, Ap. J, in press.Google Scholar
Dziembowski, W.A., Goode, P.R., Libbrecht, K.G. 1989, Ap.J., 337, L53.Google Scholar
Kuhn, J.R. 1988, Ap. J. Lett. 331, L131.Google Scholar
Libbrecht, K.G. 1989, Ap.J., 336, 1092.Google Scholar
Parker, E.N. 1987, The Internal Solar Angular Velocity, 289, Durney, B. and Sofia, S. (Eds.), Reidel, Dordrecht, The Netherlands.Google Scholar
Smirnov, A.Y. 1989, this volume.Google Scholar
Spruit, H.C. 1987, The Internal Solar Angular Velocity, 185, Durney, B. and Sofia, S. (Eds.), Reidel, Dordrecht, The Netherlands.Google Scholar
Ulrich, R.K. and Rhodes, E.J. 1983, Ap. J. 265, 551.Google Scholar