Fig. 14.
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Evolution of orbit-varying quantities for Stokes parameters. The inclination is ι = 30°. The various panels show the evolution with the orbital phase φ of the various quantities that impact the Stokes parameters: the EVPA (red), the photon’s emitted energy ω = −k ⋅ u (red, in units of the observed energy), and the sine of the emission angle sin θB (green). The left column was computed in Minkowski spacetime and the right column in Schwarzschild. The top row was computed for a vertical magnetic field and the bottom row for a toroidal field.
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