Simulation results in the form of equatorial plane cross-sections for the perpendicular (left column), intermediate (middle column), and quasiparallel (right column) simulation run. The first row a−c) shows the magnetic field, the second row d−f) the ionospheric density, the third row g−i) the stellar wind density, and the fourth row j−l) the stellar wind velocity. The x and y axes are in units of R_p. A selection of magnetic field lines have been added to a−c).