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Electron Outflow in Pulsar Magnetospheres

Published online by Cambridge University Press:  25 April 2016

R. R. Burman
R. R. Burman*
Affiliation:
Department of Physics, University of W.A.
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Extract

Mestel, Wang and Westfold (1984; ‘MWW’) have recently introduced a pulsar magnetosphere model in which electrons leave the star with non-negligible, but not highly-relativistic, speeds, and flow with moderate acceleration along magnetic field lines before reaching a limiting surface, near which rapid acceleration occurs. Such moderately accelerated flows are analysed here. A second class of flows, which do not encounter a region of rapid acceleration, is found.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 467 - 469
Copyright
Copyright © Astronomical Society of Australia 1984

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References

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Mestel, L., Wang, Y.-M., and Westfold, K. C. in preparation (1984).Google Scholar