  We perform numerical simulations in the close vicinity of a slowly rotating
young stellar object. Using our own resistive MHD Zeus347 code in 2D
axisymmetry, magnetospheric interaction experiences four robust stages in
evolution. Quasi-stationary axial and conical streams of outflowing matter can
last many orbital periods as results of the resistivity-facilitated magnetic
reconnections. The shape of the magnetic field depends on resistivity in the
magnetosphere.
