Vertical profiles of the disk density ρ, gas temperature T, radiation-to-gas pressure ratio P_rad/P_gas, and magnetic-to-gas pressure ratio P_mag/P_gas after scaling to a ﹩20 \% \,{\dot{M}}_{{\rm{Edd}}}﹩ accretion rate disk around a 10⁶ M_⊙ black hole. Angle brackets denote azimuthal averages. The vertical dotted blue lines mark the locations where the electron-scattering optical depth integrated from the disk surface reaches τ_es = 1.