Snapshot of run R1-P4-C4 (from 1 au to 10 au, with weak B_z> 0) at t = 1000T₀, showing the toroidal magnetic field in color background (blue to red), the poloidal velocity field in units of local sound speed (green arrows in the corona), and the orientation of the angular momentum flux caused by magnetic stress (purple arrows in the disk). The orientation of the angular momentum flux is reversed compared to the fiducial, accreting case.