Fig. C.1.
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Impact of Faraday effects on the Stokes parameters(ℐ, 𝒬, and 𝒰), LP, and CP evolution in a model with the vertical magnetic field viewed at i = 20deg. In the left panel, we show light curves of a model where we disabled the Faraday rotation and conversion effects by setting the Faraday rotativities to zero (radiative transfer model with ρQV = 0). In the right panels, we show the same model but with the Faraday effects taken into account. Solid and dashed lines in each subpanel indicate the model with the accretion disk and the bright spot on a clockwise (C) and counterclockwise (CC) orbit, respectively. Arrows in the 𝒬 − 𝒰 panels indicate the direction of time evolution.
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