O. Richard et al., ON THE ACCURACY OF HELIOSEISMIC DETERMINATION OF SOLAR HELIUM ABUNDANCE, Astronomy and astrophysics (Berlin), 338(2), 1998, pp. 756-760
The Helium abundance in the solar envelope is one of the most importan
t seismic observables. We investigate the accuracy of its determinatio
n taking into account uncertainties in the data and in the inversion p
rocedure. Our best value for the helium abundance in the photosphere i
s Y. = 0.248. The estimated uncertainty of 0.002 is dominated by uncer
tainties in the inversion. This does not account for possibly larger i
naccuracies in the thermodynamical data.