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Fig. 11

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Two-dimensional histograms of the discrepancy between the mean B-field orientation and the orientation inferred from the polarized dust emission, and the intensity of the polarized dust emission at three wavelengths. From left to right λ = 0.8, 1.3, and 3.0 mm. Each histogram has been constructed using the data stacked for all simulations, time-steps, and projections. The color histograms show the results using only the lines of sight that have a polarization fraction above 1%, while the gray-scale part corresponds to the rest of the points.

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