Generation of pulsar radio emission.

Details Generation of pulsar radio emission. Generation of pulsar radio emission.

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...308..809l&link_type=abstract

Astronomy and Astrophysics, v.308, p.809-820

Astronomy and Astrophysics

Astrophysics

22

Plasmas, Radiation Mechanisms: Nonthermal, Scattering, Waves, Pulsars: General

Scientific paper

The generation of radio emission from plasma waves excited by two-stream instability in pulsar magnetospheres is considered. Induced scattering transforms excited subluminal waves into superluminal ones, which escape freely in the form of transverse electromagnetic waves. The kinetics of the induced scatterings in the ulrarelativistic electron-positron plasma embedded in the superstrong magnetic field is investigated. It is shown that the spectrum and luminosity of the radio emission from plasma turbulence generated during charge density adjustment in pulsar magnetospheres are compatible with those observed.

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