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