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ИСТИНА ФИЦ ПХФ и МХ РАН |
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Based on the helioseismic inversion of the buoyancy frequency profile just below of the convective zone, we are looking for traces from the early (ZAMS) convective boundary in the hydrogen gradient profile. Specific features of the gradient profile give an estimation of depth and structure of overshooting region and a receipt for improving of the sound speed in the model.