Plasma flow nonstationarity in pulsar magnetospheres and two-stream instability

Details Plasma flow nonstationarity in pulsar magnetospheres and two-stream instability Plasma flow nonstationarity in pulsar magnetospheres and two-stream instability

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.140..325u&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 140, no. 2, Jan. 1988, p. 325-336.

Astronomy and Astrophysics

Astrophysics

25

Electron Plasma, Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Pulsar Magnetospheres, Pulsars, Electron-Positron Plasmas, Plasma Clouds, Positrons

Scientific paper

The electron-positron plasma creation near a pulsar may be a very
nonstationary process. Then, the plasma that flows out from the pulsar
environment is nonhomogeneous and gathers into separate clouds. The
dispersion of plasma clouds during the outflow, their overlapping and
the development of a two-stream instability are considered.

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