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The Equilibrium Structure of the Boundary Layer between the Magnetosphere and the Accretion Disk of an Aligned Rotator

The equilibrium structure of a magnetosphere-disk system of an accreting neutron star is calculated using a relaxation method based on the integration of the magnetohydrodynamic (MHD) equations. In a region containing the equatorial magnetopause of an aligned (counter-aligned) rotator the corotating magnetospheric plasma as well as the Keplerian disk are considered. It is shown how the magnetospheric eld enhances to support the massive thin disk. We obtain self-consistent axisymmetric solutions which are needed for future studies of the transport of plasma across the magnetospheric boundary layer by instability processes using MHD simulations.