Further improvement of the solar model.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Sun: Interior, Solar Oscillations

Scientific paper

We have improved our solar model which now has normalized differences
relative to observations laying in a band of less than 1μHz width. We
have also tested the influence of the structure of the radiative
atmosphere on the p-mode frequencies and we have found that it is
important at high frequencies.

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