Particle motion in pulsar magnetospheres

Bernd Finkbeiner, Thomas Ertl, Heinz Herold & Hanns Ruder
This report discusses some new results we found in studying the trajectories of single charged particles in the vacuum magnetosphere of a pulsar using the oblique rotator model. We believe that investigations of individual particles in the vicinity of the star can be useful for a better understanding of some fundamental problems of pulsar physics, e.g. the global structure of the magnetosphere or the pulsar radiation.
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