Vertical profiles along x = z/h(a) of the two super-A solutions shown in Fig. 5, without (left) and with (right) turbulent magnetic pressure. Top: characteristic velocities normalized to the Keplerian velocity at the disk midplane (flow speed V, modified sound speed ${\stackrel{\sim }{C}}_s$, slow and fast magnetosonic speeds V_SM, V_FM and Alfvén speed V_An). Bottom: contributions to the Bernoulli invariant E normalized to Ω_Ko²r_o²/2. The light gray area corresponds to the resistive MHD region and the vertical lines corresponds to the position of the SM and A point respectively. See text for details.