Fig. 2.
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Stokes ℐ and polarimetric images of the background accretion flow as a function of the observer’s viewing angle i and magnetic field topology. The left panel corresponds to i = 0° while i = 20°, 40°, 60°, and 80° are shown in the right panel. Total intensity and polarimetric maps are displayed in the same fashion as in Fig. 1.
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