Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere

@article{Caffau2010SolarCA,
  title={Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere},
  author={Elisabetta Caffau and Hans-G. Ludwig and M. Steffen and Bernd Freytag and Piercarlo Bonifacio},
  journal={Solar Physics},
  year={2010},
  volume={268},
  pages={255-269}
}
In the last decade, the photospheric solar metallicity as determined from spectroscopy experienced a remarkable downward revision. Part of this effect can be attributed to an improvement of atomic data and the inclusion of NLTE computations, but also the use of hydrodynamical model atmospheres seemed to play a role. This “decrease” with time of the metallicity of the solar photosphere increased the disagreement with the results from helioseismology. With a CO5BOLD 3D model of the solar… 

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