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Fig. 1

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Sketch of the geometry of the considered problem common for the MHD simulation and for the radiative transfer. The prominence slab with infinite height and length and width 2x0 is penetrated by a constant magnetic field. For a radiative transfer, we should take into account incident radiation from the surface (dashed arrows), according to the position above the solar limb (h). The line-of-sight is perpendicular to the slab.

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