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We discuss axisymmetric force-free pulsar magnetospheres with magneticallycollimated jets and a disk-wind obtained by numerical solution of the pulsarequation.  This solution represents an alternative to the quasi-spherical wind solutionswhere a major part of the current flow is in a current sheet which is unstableto magnetic field annihilation.Comment: 6 figures, accepted for publication in the Ap

Jets and Disk Winds from Pulsar Magnetospheres