Contribution to the Co-rotating Magnetic Field Model of the Pulsar

@article{Endean1970ContributionTT,
  title={Contribution to the Co-rotating Magnetic Field Model of the Pulsar},
  author={V. G. Endean and J. Allen},
  journal={Nature},
  year={1970},
  volume={228},
  pages={348-350}
}
A new general solution of the electromagnetic field equations convenient for rotating field problems is used to analyse the case of low plasma number density. Two localized pulse emitting regions rotating with the star at approximately twice the velocity of light radius are predicted. 
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