The influence of NLTE effects in Fe I lines on an inverted atmosphere - II. 6301 Å and 6302 Å lines formed in 3D NLTE

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Fig. 9.

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Effects of spectral degradation and noise on the Stokes profiles computed in 1D NLTE (black) and 3D NLTE (orange) at the five spatial positions. The differences in equivalent widths δE′ and residual intensities δI′ are computed using Eq. (4). See Sect. 4 for more details.

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