Relativistic electron distribution (top row) and emissivity (bottom row) computed from the hydrodynamic simulation at orbital phase, φ = 0.8, adopting ζ_rel = 6 × 10^-4, ζ_B = 0.5, and p = 1.2. The left and right columns correspond to points “A” and “B” in Fig. 9. Note that Inverse Compton cooling causes an increase in the emissivity at lower frequencies in this case. Furthermore, the curves for the calculations with Coulomb cooling in the emissivity plots are closely associated with those for the intrinsic emission.