Polarization angle (Ψ), summed between 2 and 8 keV, as a function of the inclination of the source, for models consistent with the constraints from IXPE analyses and BLR reverberation studies. For all models shown, the coronal temperature is set to kT_e = 60 keV and the coronal inner radius is set to the ISCO radius corresponding to the BH spin (R_corona = 6R_G when a = 0 and R_corona = 1.24R_G when a = 0.998).