Vertical profiles along x = z/h of the two super-SM solutions shown in Fig. 2, without (left) and with (right) turbulent magnetic pressure. From top to bottom: gas P, laminar horizontal P_lam = (B_r² + B_ϕ²)/2μ_o and turbulent P_turb magnetic pressures; velocity components u_i (normalized to Keplerian speed Ω_K0r₀); electric current densities J_i (normalized to B_zo/μ_oh); laminar magnetic field components B_i (normalized to B_zo). The light gray area corresponds to the resistive MHD region and the vertical line corresponds to the position of the SM point. Note that α_P = 0 requires μ = 0.6, while α_P = 2 requires μ = 3.9. See text for more details.