a)–c) Ambiguity resolved azimuths in local solar coordinates, Φ, at log (τ) = 0, − 0.9 and −2.3from left to right. North is up and corresponds to an angle of 90°. West is to the right and corresponds to an angle of 0°. d)–f) The local solar coordinate corrected inclinations, Γ, of the magnetic field after the azimuth ambiguity resolution at log (τ) = 0, − 0.9 and −2.3from left to right. The inclinations and azimuths of pixels with B< 300 G at log (τ) = −2.3 and B< 700 G at log (τ) = 0 and −0.9 are shown in white.