Composition and Opacity in the Solar Interior |
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| Authors: | Sylvaine Turck-Chieze |
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| Institution: | (1) CEA/DSM/DAPNIA/Service d'Astrophysique, CE Saclay, 91191 Gif-sur-Yvette Cedex 01, France |
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| Abstract: | 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.
This revised version was published online in June 2006 with corrections to the Cover Date. |
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