Escaping Radio Emission from Pulsars: Possible Role of Velocity Shear

Details Escaping Radio Emission from Pulsars: Possible Role of Velocity Shear Escaping Radio Emission from Pulsars: Possible Role of Velocity Shear

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...479l.129m&link_type=abstract

Astrophysical Journal Letters v.479, p.L129

Astronomy and Astrophysics

Astronomy

23

Plasmas, Stars: Pulsars: General, Waves

Scientific paper

It is demonstrated that the velocity shear, intrinsic to the e+e- plasma present in the pulsar magnetosphere, can efficiently convert the nonescaping longitudinal Langmuir waves (produced by some kind of a beam or stream instability) into propagating (escaping) electromagnetic waves. It is suggested that this shear-induced transformation may be the basic mechanism needed for the eventual generation of the observed pulsar radio emission.

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