Four typical geometries in our solutions: Disk+Column (DC), Disk (D), Disk+Column+Ejection1 (DCE1), and Disk+Column+Ejection2 (DCE2) illustrated by snapshots in quasi-stationary states in simulations b8, d12, b5, and c9 (top to bottom, respectively). We show the density in a logarithmic color grading, with a sample of magnetic field lines in red solid lines. White lines labeled a, a’, b, and c delimit the components of the flow between which we integrate the fluxes; R_in, R_out and R_cor are the inner disk edge, the furthest outer reach of closed stellar field in the disk and the corotation radius, respectively.