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Fig. 1.

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Sample of Stokes spectra synthesized from the extracted atmospheric models of different solar features. Panels a-c: stratification of the temperature (a), LOS velocity (b), and magnetic field strength (c) from one pixel for each atmospheric feature taken from the sample of extracted atmospheres. Panel d: the continuum intensity from the MHD cube at 4015 Å with extracted atmospheres annotated with yellow dots. Panels e-h: Stokes parameters in the 4015–4017 Å spectral range from the atmospheres displayed in panels a-c. Wavelengths are given with respect to 4016 Å. For easier comparison, the Stokes profiles are normalized to the local continuum intensity Ic and the Stokes I/Ic profiles from different features are shifted vertically.

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