Plasma processes in pulsar magnetospheres and eclipsing binary pulsar systems.

Details Plasma processes in pulsar magnetospheres and eclipsing binary pulsar systems. Plasma processes in pulsar magnetospheres and eclipsing binary pulsar systems.

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998brjph..28..191q&link_type=abstract

Braz. J. Phys., Vol. 28, No. 3, p. 191 - 202

Physics

Pulsar Magnetospheres: Plasma, Pulsar Magnetospheres: Radiation Mechanisms, Binary Pulsars: Eclipses

Scientific paper

Plasma processes that may be responsible for pulsar radio emission and for eclipses observed for binary pulsars are discussed. The high brightness temperature of pulsar radio emission implies that the radiation mechanism must be coherent. Several emission mechanisms are discussed. The high brightness temperature of radio emission also implies that a nonlinear effect on wave propagation through pulsar magnetospheric plasmas is important and may result in radio pulse microstructure or cause fluctuations in dispersion measure. The discovery of eclipsing binary pulsars provides an opportunity to study nonlinear wave-wave interactions in electron-ion plasmas in the winds (or magnetospheres) of companion stars.

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