Field strength, inclination, and azimuth maps resulting from the inversion of the observed Stokes profiles with the HAZEL code. Each column represents one of the two 90° ambiguous solutions, quasi-horizontal (left) and quasi-vertical (right). As in Fig. 1, the black bottom region represents the solar disk. The rest of the dark areas correspond to pixels whose Stokes Q/I and U/I signals did not exceed 5 times their corresponding noise levels.