Comment on "Self-Consistent Solution for an Axisymmetric Pulsar Model"

Details Comment on "Self-Consistent Solution for an Axisymmetric Pulsar Model" Comment on "Self-Consistent Solution for an Axisymmetric Pulsar Model"

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974phrvl..33.1521m&link_type=abstract

Physical Review Letters, vol. 33, Issue 25, pp. 1521-1523

Physics

4

Scientific paper

The numerical results of Kuo-Petravic, Petravic, and Roberts, in which magnetic field lines are found to close beyond the light cylinder, are reconciled with the canonical theoretical view that these field lines must be open. We argue that a small region of trapped plasma on closed field lines relatively near the star (but nevertheless outside of it) expands until the light cylinder is reached. The remaining field lines are forced open and do not close beyond the light cylinder.

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