Fig. 1.
Different solar atmosphere models and corresponding synthetic Stokes I profiles. Panel a: temperature against the continuum optical depth at λ = 500 nm for the three solar atmosphere models. Panels b, c: synthetic Stokes I profiles of the Mg I 12.32 μm and Mg I 12.22 μm without magnetic fields. The relative intensity profiles are relative to the continuum intensity in the corresponding model.
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