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The Convection Zone and Oscillations
Published online by Cambridge University Press: 08 February 2017
Extract
We study the influence of the structure and physics of the uppermost superadiabatic layers on the oscillation spectrum of p-modes. These modes are trapped inside the Sun by reflecting at the upper layers of the Sun, so these layers are important for the oscillation spectrum. Indeed, the main difference between the computed and observed frequencies seems to come from these layers (Christensen-Dalsgaard, 1985; Christensen-Dalsgaard and Thompson, 1997).
- Type
- II. Solar Convection and Variation of Irradiance
- Information
- Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 85 - 88
- Copyright
- Copyright © Kluwer 1998