Fig. 3

Probability density functions (PDFs) of a) the intrinsic field strength, B, b) the magnetic filling factor, α and c) the inclination γ of the pixels having Bapp,los in an interval of ± 200 G around the peak value of Bapp,los, for the quiet Sun (dotted curves) and the active region (solid curves) fields of view shown in Fig. 1. The vertical lines mark the mean values of the distributions.
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