We model the submillimeter patterns that are expected for filamentary clouds that are threaded by helical magnetic fields. We previously developed a three-parameter model of such clouds, which are described by a concentration parameter C and two flux-to-mass ratios Γz and Γ to specify the mass loading of the poloidal and toroidal field lines, respectively. Our models provide a simple and purely geometric explanation for the well-known polarization hole effect, in which the submillimeter percentage decreases toward the regions of peak intensity. This occurs because of a cancellation between contributions to the from the backbone of poloidal flux along the filament's axis and its surrounding envelope, which is dominated by the toroidal field component. A systematic exploration of our parameter space allows us to classify the patterns due to filaments aligned approximately perpendicular to the plane of the sky into three basic types. The vectors are parallel to filaments when Bz,S/B,S 0.1, where Bz,S and B,S are, respectively, the poloidal and toroidal magnetic field components at the outer surface of the filament. The vectors are perpendicular to filaments when Bz,S/B,S 0.37. Intermediate cases result in patterns that contain 90° flips in the orientation of the vectors. The flips are symmetric about the central axis for filaments oriented parallel to the plane of the sky, but more complicated asymmetric patters result from filaments that are inclined at some angle.
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