Three‐dimensional Simulations of Disk Accretion to an Inclined Dipole. I. Magnetospheric Flows at Different Θ

We present results of fully three-dimensional MHD simulations of disk accretion to a slowly rotating magnetized star with its dipole moment inclined at an angle Θ to the rotation axis of the disk (which is aligned with the spin axis of the star). The main goal was to investigate the pattern of magne... View More