Pulsar-magnetosphere plasma

Details Pulsar-magnetosphere plasma Pulsar-magnetosphere plasma

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986svjpp..12.1233l&link_type=abstract

Fizika Plazmy (ISSN 0367-2921), vol. 12, Oct. 1986, p. 1233-1249. In Russian.

Physics

2

Dense Plasmas, Electrostatic Waves, Neutron Stars, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Electron Plasma, Electron-Positron Plasmas, Field Strength, Relativistic Particles, Stellar Magnetic Fields

Scientific paper

An attempt is made to describe, from a unified standpoint, the fundamental physical processes underlying the generation of pulsar radiation. The neutron star magnetosphere must contain a dense plasma consisting of an electron-positron plasma pierced by a relativistic particle beam. Such a plasma is thought to be the most probable source of pulsar radiation. The linear properties of waves in an electron-positron plasma with a strong magnetic field are analyzed. The possible instabilities of the pulsar-magnetosphere plasma are examined from the standpoint of pulsar activity.

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