A cylindrical pulsar magnetosphere model with particle inertia

Details A cylindrical pulsar magnetosphere model with particle inertia A cylindrical pulsar magnetosphere model with particle inertia

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aujph..32..681b&link_type=abstract

Australian Journal of Physics, vol. 32, Dec. 1979, p. 681-693. Research supported by the Science Research Council.

Physics

6

Cosmic Plasma, Particle Motion, Pulsar Magnetospheres, Pulsars, Stellar Models, Stellar Rotation, Electromagnetic Fields, Equations Of Motion, Inertia, Particle Trajectories, Plasma Dynamics

Scientific paper

An investigation is made of the equations to a steadily rotating nonaxisymmetric pulsar magnetosphere model, with the effects of particle inertia fully incorporated but with no dissipative forces. As an illustrative example the basic theory is applied to a 'cylindrical pulsar' model, in which quantities do not vary parallel to the rotation axis. It is shown that Endean's Bernoulli-type integral imposes severe constraints on particle motion, indicating that, in a realistic model, dissipation (e.g. by radiation damping) may play an essential role.

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