  Selfconsistent magnetospheres of rotating cosmic magnets (neutron
stars/pulsars) with arbitrary inclination of the magnetic against the rotation
axis are considered. Present studies concentrate on the regime dominated by the
force--free surface (FFS). A macroscopic fluid description is applied and
radiation reaction is taken into account. As in earlier work of our group, a
'standard set of parameters' is used. Under these conditions, the following
features are found among other results: global charge separation exists for all
degrees of inclination of the magnetic against the rotation axis; clouds of
different charge are seperated by regions of vanishing particle number density;
as expected, test particles inserted into the latter regions propagate into one
of the adjacent clouds; strong polodial currents exist; locally averaged
particle energies for protons typically range up to $10^{16}-10^{17}$ eV,
depending on the angle of inclination.
