Seismic calibration of the solar envelope model

Details Seismic calibration of the solar envelope model Seismic calibration of the solar envelope model

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..615b&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Physics

3

Helioseismology

Scientific paper

With extensive and accurate p-mode data now available, we reconsider the problem of seismic calibration of the adiabatic part of the solar convective envelope, including the measurement of the He abundance and of the specific entropy, and testing the equation of state. Our approach is based on the direct fitting using the multiparametric families of envelope models and the differential-response technique, which allows transferring the surface boundary conditions of the oscillation equations downwards, to eliminate the uncertain effects of the near-surface layers.

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