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Fig. 2

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Stokes Q polarization maps obtained for filaments (left) and sheets (right) with different parameter values for the stochastic component of the magnetic field Bsto. The component amplitude (ni) is constant in column and increases from left to right, and the correlation length (nc) is constant in rows and increases from top to bottom. The circular regions, here centered on the north Galactic pole, have an angular radius of 12.53°. The shape parameters, including those controlling the wiggles, are the same as in Fig. 3 and are kept fixed between panels. All maps share the same color scale.

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