Strong Langmuir turbulence and the pulsar emission mechanism

Details Strong Langmuir turbulence and the pulsar emission mechanism Strong Langmuir turbulence and the pulsar emission mechanism

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..291a&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 291-294 (SEE N89-24910 18-75)

Astronomy and Astrophysics

Astrophysics

Plasma Turbulence, Pulsars, Radio Emission, Stellar Radiation, Plasma Interactions, Plasma Waves, Wave Propagation

Scientific paper

The pulsar emission mechanism based on the plasma beam interaction is examined. The linear study shows that, due to obliquity of wave propagation and to magnetic field line curvature, the resulting unstable Langmuir waves have simultaneously electrostatic and electromagnetic features. The nonlinear analysis produces Langmuir solitons with associated electromagnetic features in a quite natural way. These features are compared to the characteristics of observed pulsar radio emission.

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