Toroidal magnetic field values along the disk surface (top) and along the disk height (measured from the disk equatorial plane) at R = 12R_⋆ (bottom) are shown in terms of their dependence of stellar rotation rates. The values are averaged over 10 stellar rotation periods during the quasi-stationary states, in the cases with α_m = 1 and B_⋆ = 500 G (simulations b1, b5, b9, and b13). In black, green, blue, and red dashed lines we display the values for 0.05, 0.1, 0.15, and 0.2 of Ω_br, respectively. The black solid lines provide the reference for typical radial and vertical dependence.