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Sensitivity of solar p-modes to solar envelope structure
Published online by Cambridge University Press: 03 August 2017
Abstract
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