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On the implications of the symmetric component of the frequency splitting reported by Duvall, Harvey and Pomerantz

Published online by Cambridge University Press:  03 August 2017

D.O. Gough
Affiliation:
Institute of Astronomy and Department of Applied Mathematics and Theoretical Physics, University of Cambridge, UK
M.J. Thompson
Affiliation:
Institute of Astronomy and Department of Applied Mathematics and Theoretical Physics, University of Cambridge, UK

Abstract

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The component of the frequency splitting of solar five-minute oscillations observed by Duvall, Harvey and Pomerantz that is even in azimuthal degree measures latitudinal and depth variations in the structure of the sun. We indicate how the data hint that there is a shallow perturbation, possibly associated with a magnetic field, that is concentrated at low latitudes.

Type
Chapter 2: Theory of Solar Oscillations
Copyright
Copyright © Reidel 1988 

References

Bogdan, T.J. and Zweibel, E.G. 1985 Astrophys J. 298, 867875 CrossRefGoogle Scholar
Duvall, T.L. Jr, Harvey, J.W. and Pomerantz, M.A. 1986 Nature 321, 500501 CrossRefGoogle Scholar
Gough, D.O. 1986 Hydrodynamic and hydromagnetic problems in the sun and stars (ed. Osaki, Y., Univ Tokyo) 117143 Google Scholar
Tarbeil, D.T., Title, A.M. and Schoolman, S.A. 1979 Astrophys. J., 229, 387392 CrossRefGoogle Scholar