Solar models with a helioseismic sound speed profile

Physics

Scientific paper

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Scientific paper

The problem of computation of the present Sun model with a given sound speed profile in the solar radiation zone is considered. It is shown that the chemical composition is still a free parameter, but the entropy of the adiabatic part of the convective zone is determined by the simulation procedure. The parameters of the models are compared with the helioseismic calibration of the solar envelope and a disagreement is revealed. Study of the seismic properties of the model cores indicates that the best model shows closeness to the standard solar model.

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