The seismic solar model as the state-of-the-art model of the sun

Details The seismic solar model as the state-of-the-art model of the sun The seismic solar model as the state-of-the-art model of the sun

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999adspr..24..181t&link_type=abstract

Advances in Space Research, Volume 24, Issue 2, p. 181-184.

Computer Science

Sound

3

Scientific paper

We determine the structure of the solar interior subject to the constraints on the sound speed profile, the density profile, and the depth of the convection zone, all of which are obtained by the helioseismic inversion. We do not a priori assume the chemical composition profiles but obtain them as part of our solutions. This means that we do not have to follow the evolution of the Sun. The determined seismic solar models are more suitable for the discussion of the solar neutrino problem than the conventional standard solar models because the seismic solar models are completely consistent with helioseismology while the standard solar models are not.

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