Helioseismology and standard solar models

Details Helioseismology and standard solar models Helioseismology and standard solar models

1996-12-05

arxiv.org/abs/astro-ph/9612053v1

Astropart.Phys. 7 (1997) 77-95

Astronomy and Astrophysics

Astrophysics

16 pages, 4 tables and 5 ps figures, uses tighten.sty, aps.sty and revtex.sty

Scientific paper

10.1016/S0927-6505(97)00004-2

We present a systematical analysis of uncertainties in the helioseismological determination of quantities characterizing the solar structure. We discuss the effect of errors on the measured frequencies, the residual solar model dependence and the uncertainties of the inversion method. We find Y_{ph}=0.238-0.259, $R_b/R_\odot=0.708-0.714$ and $\rho_b=(0.185-0.199)$ gr/cm^3 (the index b refers to the bottom of the convective envelope). In the interval $0.2

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