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Sensitivity of solar p-modes to solar envelope structure

Published online by Cambridge University Press:  03 August 2017

P. Demarque  and
D. B. Guenther
P. Demarque
Affiliation:
Center for Solar and Space Research, Yale University, P.O. Box 6666, New Haven, CT 06511, USA
D. B. Guenther
Affiliation:
Center for Solar and Space Research, Yale University, P.O. Box 6666, New Haven, CT 06511, USA

Abstract

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We present a study of the effects of diffusion of helium and heavy elements from the convection zone into the radiative layer immediately below the convection zone, on the structure of the solar envelope. A comparison is made of the p-mode oscillation spectrum and the run of the speed of sound in a model with diffusion, in a standard model, and with observation.

Type
Chapter 2: Theory of Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 91 - 94
Copyright
Copyright © Reidel 1988 

References

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