Mechanism for the radio emission of pulsars

Details Mechanism for the radio emission of pulsars Mechanism for the radio emission of pulsars

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986zhpmr..44...18b&link_type=abstract

(ZHETF Pis'ma v Redaktsiiu, vol. 44, July 10, 1986, p. 18-20) JETP Letters (ISSN 0021-3640), vol. 44, July 10, 1986, p. 20-23. T

Physics

Dielectrics, Electrodynamics, Magnetohydrodynamic Flow, Pulsars, Radio Emission, Relativistic Plasmas, Airy Function, Electron-Positron Plasmas, Magnetospheres, Neutron Stars, Plasma Density

Scientific paper

An instability of the flow of a relativistic electron-positron plasma in
a strong curvilinear magnetic field is predicted theoretically. This
instability can explain the origin and basic properties of the observed
radio emission of pulsars.

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