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

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997uta..rept.....m&link_type=abstract

Technical Report, DOE/ER/54346-772; IFSR-772; DE97-005271 Inst. for Fusion Studies

Physics

Pulsars, Plasmas (Physics), Radio Emission, Electromagnetic Radiation, Longitudinal Waves, Pulsar Magnetospheres

Scientific paper

It is demonstrated that the velocity shear, intrinsic to the e+e(minus) 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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