Statistics – Computation
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.196..101m&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 196, no. 1, p. 101-107.
Statistics
Computation
3
Electron-Positron Plasmas, Electrostatic Waves, High Temperature Plasmas, Plasma Drift, Pulsar Magnetospheres, Rotating Plasmas, Computational Astrophysics, Vortices
Scientific paper
Electrostatic drift wave in a hot rotating and strongly magnetized electron-positron pulsar plasma is considered. Using relativistic two-fluid equations a pair of coupled nonlinear equations is derived. It is shown that the wave can propagate in the form of 2D dipolar vortices at ultrarelativistic temperature of the plasma. The latter may affect the energy transport in the hot plasma, which can lead to a new turbulent state in the pulsar magnetosphere.
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