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

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

Oct 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.228..348e&link_type=abstract

Nature, Volume 228, Issue 5269, pp. 348-350 (1970).

Physics

17

Scientific paper

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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