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.
Fecha de publicación:
4
2001