Horizontal (in the τ₅₀₀₀ depth scale) cuts of several interesting physical parameters in the multi-cube resulting from the inversion, including the NLTE correction. The left column shows the temperature in kK at three different heights. The top row also shows the line-of-sight magnetic flux density (middle panel) in G and the transverse (on the plane of the sky) magnetic flux density (right panel) at the base of the photosphere. The middle row shows the variation in the flux density from log (τ₅₀₀₀)  = 0 to log (τ₅₀₀₀)  = −1 (middle panel: line-of-sight component; right panel: transverse component). The bottom row shows the variation in the temperature in kK (middle panel) and the line-of-sight velocity in km s^-1 (right panel) from log (τ₅₀₀₀)  = 0 to log (τ₅₀₀₀)  = −1 inside the magnetic atmosphere.