000001950 001__ 1950
000001950 005__ 20160701171656.0
000001950 0247_ $$2DOI$$a10.1016/S0273-1177(02)00170-9
000001950 037__ $$aASTROimport-107
000001950 100__ $$aGrevesse, N.
000001950 245__ $$aThe Composition of the solar photosphere
000001950 260__ $$c2002
000001950 520__ $$aThe Sun is unique because chemical composition data can be derived from very different layers, from the center to the outermost coronal layers, using very different techniques like helioseismology, spectroscopy, particle collection techniques, … Differences in chemical composition are observed allowing to discover how the different solar layers evolve. The composition of the solar photosphere, which represents the composition of the outer convective zone, is the basic reference source of elemental abundances. We review the current status of our knowledge of the chemical composition of this layer and compare it with data from other solar sources as well as with meteoritic data. 
000001950 700__ $$a Sauval, A. J.
000001950 773__ $$c3-11$$i1$$pAdvances in Space Research$$v30$$y2002
000001950 85642 $$ahttp://esoads.eso.org/abs/2002AdSpR..30....3G
000001950 905__ $$apublished in
000001950 980__ $$aREFERD