2D profiles of temperature and the irradiation heating term for the hydrostatic model at i = 30 iterations. The orange line refers to the τ_⋆ = 1 profile for the stellar radiation using the Planck mean opacity. Blue lines refer to τ_ν = 1 profiles for for different frequencies ν (same as in Fig. 2), with the line opacity weighted by B_ν at that frequency. (see also Fig. 7 in Melon Fuksman & Klahr 2022). The red line indicates the τ_disk = 1 profile for the disk’s radiation using κ_P(T). The green lines indicate the midplane gas scale height of the disk.