On the relation of the Duvall phase function to the upper layers on the convection zone
A method to obtain the Duvall phase function from the structure of a stellar model is presented. This can be a good tool for understanding the dependence of p-mode frequencies on the structure of the upper layers of the convection zone. A linear relation between phase function differences of two models and their equilibrium structure differences is
Christensen-Dalsgaard, J. et al.
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12
1988