Composition and Opacity in the Solar Interior

Details Composition and Opacity in the Solar Interior Composition and Opacity in the Solar Interior

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ssrv...85..125t&link_type=abstract

Space Science Reviews, v. 85, Issue 1/2, p. 125-132 (1998).

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9

Scientific paper

Detailed abundances of elements from hydrogen up to iron are necessary
to perform a precise model of the solar structure. Most of them have
been deduced from photospheric observed values, some others from the
meteoritic composition. Nowadays, thanks to helioseismic constraints,
they seem more and more under control.

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