Excitation of plasma turbulence in pulsar magnetospheres

Details Excitation of plasma turbulence in pulsar magnetospheres Excitation of plasma turbulence in pulsar magnetospheres

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993astl...19...14l&link_type=abstract

Astronomy Letters, Vol. 19, p. 14-18; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 19, no. 1, p. 34-44. In Russian.

Physics

7

Electron-Positron Plasmas, Plasma Turbulence, Pulsars, Stellar Magnetic Fields, Stellar Winds, Magnetohydrodynamic Stability, Radio Emission, Stellar Physics

Scientific paper

Maintenance of the self-consistent charge and current distribution in a pulsar plasma, streaming away along the open magnetic field lines, is considered. It is shown that a small fraction of particles should stream toward the main plasma flow. Therefore the two-stream instability generates plasma oscillations that may be a source of pulsar radio emission.

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