Fig. 3
Distribution of grain sizes aalg, where dust particle start to align to the magnetic field direction B according to RAT theory. The plane shown is perpendicular to the mid-plane of the disks. The disk model D03 with 10-3 M⊙ is in the left panel and the model D05 with 10-5 M⊙ is in the right panel. Lower values of aalg result in higher degrees of linear polarization.
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