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Fig. 1.


Examples of three simulated Stokes profiles as RTE is solved for a snapshot of the Rempel simulation of a sunspot (Rempel 2012). Top panel: monochromatic continuum intensity map in which three pixels are highlighted in black, red, and light-blue squares as representatives of low magnetized, penumbral, and umbral areas, respectively; their spectral profiles are presented following this same color code in panels a–d for Stokes I,  Q,  U, and V, respectively. The physical parameters (T(z), Pg(z), ρ(z), vLOS(z), Bx(z), By(z), and Bz(z)) that lead to these profiles are shown in panels e–k, respectively.

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