Cyclotron instability and radio emission generation in pulsar magnetospheres

Details Cyclotron instability and radio emission generation in pulsar magnetospheres Cyclotron instability and radio emission generation in pulsar magnetospheres

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..910m&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Oct. 1989, p. 910-917. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

6

Cyclotron Radiation, Pulsar Magnetospheres, Radio Emission, Electron-Positron Pairs, Electron-Positron Plasmas, Magnetic Field Configurations, Stellar Magnetic Fields

Scientific paper

It is shown that cyclotron instability can develop in the magnetosphere of a typical pulsar if the magnetic field structure near its surface differs significantly from the dipolar one so that the radius of curvature of the magnetic field lines is of the order of a radius of the neutron star. The cyclotron instability develops in the neighborhood of the pulsar's light cylinder leading to the generation of a radio emission. The characteristics of this emission are discussed.

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