Equations for pulsar magnetospheres with particle inertia

Details Equations for pulsar magnetospheres with particle inertia Equations for pulsar magnetospheres with particle inertia

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978aujph..31..455b&link_type=abstract

Australian Journal of Physics, vol. 31, no. 5, Oct. 1978, p. 455-458. Research supported by the Science Research Council of Eng

Physics

7

Flow Equations, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Stellar Models, Bernoulli Theorem, Inertia, Plasma Dynamics, Relativistic Plasmas, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

This note deals with steadily rotating nonaxisymmetric pulsar magnetospheres, with the effects of particle inertia fully incorporated. It is pointed out that the equations of motion for the component species of a relativistically streaming nondissipative plasma can be considerably simplified by using the steady-rotation constraint together with a fluxoid conservation law and Endean's Bernoulli-type integral.

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