Azimuthally-averaged temperature profiles for four pairs of models, showcasing influence of each of four variables in our parameter space (M_p, Ṁ, α, r_p) on spiral shock heating. Our fiducial model (M_p = 100 M_⊕, Ṁ = 10⁻⁸, α = 10⁻³, r_p = 4) is shown in blue on every panel, while dashed lines depict initial profiles of the model of corresponding color. In all cases, we noted stronger shock heating in optically thicker regions of the disks. This behavior can also be seen in the rest of our suite of models.