Illustration of the regions in which the mass fluxes were measured. We calculate the jet mass-loss rate, MF Jet, along the blue line, where the velocity field is directed outward, and the magnetospheric mass-accretion rate, MF Mag, along the red line, where the velocity field is directed inward. The star is represented in yellow. The gray area extends from the surface of the star to r_o, where integration starts. The magnetospheric region is delimited by the closed magnetic fieldlines (solid black lines), at the initial stage of the MHD simulations.