Radiation from Flares near the Magnetic Poles of Pulsars

Details Radiation from Flares near the Magnetic Poles of Pulsars Radiation from Flares near the Magnetic Poles of Pulsars

May 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.237..157g&link_type=abstract

Nature, Volume 237, Issue 5351, pp. 157-158 (1972).

Physics

4

Scientific paper

IT is generally accepted that pulsar emission is produced by material ejected from the surface of rotating neutron stars near the magnetic poles. The charged particles are thought to radiate as they are accelerated along magnetic field lines or as they approach the ``speed of light cylinder''. But the exact mechanisms by which emission is produced over the full range of the spectrum from gamma rays to radio frequencies1,2 are not understood.

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