Histograms of the inferred field vector (strength, inclination, and azimuth) and the filling factors using a model with two magnetic atmospheres contaminated by 30% of unpolarised stray light. All the inverted pixels have Stokes Q or U or V signals above 4σ_n and have better fits than the single magnetic component inversion. The blue (red) lines represent the large (small) component, the one with larger (smaller) filling factor. The dotted grey lines superposed to the inclination histogram represent a sinθ distribution. Taking into account that the azimuth is uniform, these dotted lines represent an isotropic distribution of the field vector.