Polarized images. Top panels: calculated images B₀, B₆₀, and B₁₂₀ denoting the corona observed with different orientations of the polarizers. The logarithmic color scale corresponds to the scale from Fig. 2. Bottom panels: radial (left) and polar (right) profiles. For reference, we plot the total brightness B, as well as the brightness of the eclipse K corona, the solar limb, and the vignetting zone.