The Iron Line Formation Problem in Three-dimensional Hydrodynamic Models of Solar-like Photospheres
            
    This paper presents the results of a detailed theoretical investigation of the iron line formation NLTE problem in a three-dimensional model of the solar photosphere, which we have obtained from a very recent radiation hydrodynamics simulation of solar surface convection. In this first paper we have neglected the effects of horizontal radiative
            Shchukina, Nataliya et al.
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                        2001