2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/181310We discuss axisymmetric force-free pulsar magnetospheres with magnetically collimated jets and a disk-wind obtained by numerical solution of the pulsar equation. This solution represents an alternative to the quasi-spherical wind solutions where a major part of the current flow is in a current sheet which is unstable to magnetic field annihilation.6 figures, accepted for publication in the ApJAstrophysicstext