Two-stream instability in pulsar magnetospheres

Details Two-stream instability in pulsar magnetospheres Two-stream instability in pulsar magnetospheres

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..257u&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 257-260 (SEE N89-24910 18-75)

Physics

Plasma Physics

Magnetohydrodynamic Stability, Pulsars, Radio Bursts, Stellar Magnetospheres, Stellar Radiation, Electron Plasma, Plasma Physics, Space Plasmas, Stellar Magnetic Fields

Scientific paper

Reasons that could produce two-stream instability in pulsar plasma are discussed. It is noted that if the outflow of electron-positron plasma from the pulsar vicinity is stationary, this instability either is stabilized, or its growth rate is so low that the plasma leaves the pulsar magnetosphere before the instability is developed. The electron-positron plasma creation near a pulsar may be a very nonstationary process. If this nonstationarity is accounted for, the situation radically changes allowing the two-stream instability development in the pulsar plasma.

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