Grevesse, N. ; Sauval, A. J.

published in Space Science Reviews, 85, pp. 161-174 (1998)

Abstract: We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic abundances confirms that there is a very good agreement between the two sets of abundances. They are used to construct a Standard Abundance Distribution.

DOI: 10.1023/A:1005161325181
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