Magnetic field strength B(x,y,log τ₅ = 0) (left) and vertical component of the magnetic field in the local reference frame B_z(x,y,log τ₅ = 0) (right) in NOAA 12049 observed on May 3, 2014 at Θ = 6.5°. White contours in the left and right panels indicate regions where B< 500 Gauss and B_z< 0, respectively. Black arrows indicate the projection of the magnetic field vector B onto the plane of the solar surface. This region corresponds to the red rectangle in Fig. 1 (bottom panel). This map was obtained from inverting the deconvolved data assuming p_w = 0.2 (20% wide-angle scattered light).