Fig. 5.
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Spectra (top row) and PD (bottom row) of the disk radiation at the emission at different inclinations with respect to the disk normal, θ = 13° (cyan), 39° (orange), 55° (green), 68° (red), and 80° (purple), considering two values of the BH spin, a = 0 (left column) and 0.998 (right column). A BH mass of M = 10 M⊙ and accretion rate of 0.1 ṀEdd were set, with a hardening factor of fcol = 1.8 and a stop column density of NH = 1024 cm−2. The disk medium is modeled in either the CIE (dotted lines) or the PIE (solid lines) regimes. The Stokes parameters for radiation emitted from each radial bin are weighted according to the temperature and area of each bin (see Equations 5).
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