Electron Outflow in Pulsar Magnetospheres
1984 ◽
Vol 5
(4)
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pp. 467-469
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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.
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1996 ◽
Vol 160
◽
pp. 433-434
1996 ◽
Vol 160
◽
pp. 409-416
Keyword(s):
2012 ◽
Vol 8
(S291)
◽
pp. 552-554
1992 ◽
Vol 128
◽
pp. 112-113
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2000 ◽
Vol 12
(2)
◽
pp. 145-153
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1990 ◽
Vol 44
(1)
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pp. 25-32
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