Results from the multi-line inversions of the VTT observations. Top to bottom: temperature T_inv, magnetic field strength B_inv, magnetic field inclination γ_inv, and LOS velocity v_inv. Left to right: different optical depths log τ = 0, −1, and −2. The white or black contours correspond to a magnetic field of 1000 G and were used to highlight the sunspot and pore. These contours serve as a mask for the inclination maps, showing only the inferred values for the sunspot and the pore, where the results are more reliable. The cross and diamond symbols show the location of the pixels plotted in Figs. 9 and 10.