Vertical structure of the disk-corona system computed at the single radius R = 10 R_Schw for ṁ = 0.05. The horizontal axis is the height above the disk midplane given in scale height H defined by Eq. (36). Three significant locations are marked with vertical dotted lines: the photosphere (green), the temperature minimum (dark yellow), and the thermalization depth (red). The following panels display (a) radiation and gas temperature; (b) gas, radiation, magnetic, and total pressure; (c) gas density and pressure gradients; (d) radiative energy flux, magnetic (Poynting) flux, and gas heating rate all normalized to the total accretion flux F_acc; (e) net radiative cooling terms (Λ_B and Λ_C) and gas magnetic heating rates; and (f) electron scattering and total and effective optical depths.