Latitudinal profiles (zoomed in on the disk) of thermal pressure, P; laminar (total) magnetic pressure, P_lam; turbulent magnetic pressure, P_turb (all normalized to P at the disk midplane); components of the magnetic field, B_R, B_θ, and B_ϕ (normalized to B_z at the disk midplane); and components of the velocity, v_R, v_θ, and v_ϕ (normalized to the Keplerian velocity, v_K, at the disk midplane) from three numerical (solid lines) and theoretical (dashed) solutions. The shaded regions correspond to the disk (light gray for the numerical solution and dark gray for the semi-analytical one), and the vertical lines mark the transition to the ideal MHD regime (solid lines for the simulations and dashed lines for the semi-analytical solutions).