Abstract
A new value of the ratio of the heavy elements content to hydrogen abundance Z/X has been recently estimated in the solar atmosphere. We present the consequences of this result on the solar standard model and we examine the sensitivity to Z/X of the solar neutrinos flux predictions and of the oscillation frequencies.
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© 1995 Springer-Verlag
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Morel, P., Berthomieu, G., Provost, J., Lebreton, Y. (1995). About solar model calibration. In: Roxburgh, I.W., Masnou, JL. (eds) Physical processes in astrophysics. Lecture Notes in Physics, vol 458. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0118716
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DOI: https://doi.org/10.1007/BFb0118716
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