Jets and Disk-Winds from Pulsar Magnetospheres
  We 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. 
Richard V.E. Lovelace, Leaf Turner, Marina M. Romanova