Current adjustment in pulsars

Details Current adjustment in pulsars Current adjustment in pulsars

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...261..544l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 2, p. 544-550.

Statistics

Computation

21

Computational Astrophysics, Electron-Positron Plasmas, Pulsar Magnetospheres, Current Density, Magnetohydrodynamic Flow, Plasma Turbulence, Radio Emission, Stellar Rotation

Scientific paper

Longitudinal current in pulsar magnetospheres must be adjusted for the global magnetospheric structure. The required current density may be generated in electron-positron discharge only if a certain flow of particles (electrons or positrons) falls to the discharge from above. Counterstreaming plasma flows in the magnetosphere cause plasma turbulence; this may be relevant to the problem of pulsar radio emission.

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