The emergence of electromagnetic waves from pulsar magnetospheres

Details The emergence of electromagnetic waves from pulsar magnetospheres The emergence of electromagnetic waves from pulsar magnetospheres

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pazh....8..685m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Nov. 1982, p. 685-688) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Nov.-Dec.

Astronomy and Astrophysics

Astronomy

6

Electromagnetic Wave Transmission, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Stellar Magnetic Fields, Cyclotron Resonance, Damping, Electron Plasma, Electron-Positron Plasmas, Nonuniform Magnetic Fields, Positrons, Relativistic Plasmas

Scientific paper

In relativistic electron-positron plasma subject to a longitudinally nonuniform, curvilinear magnetic field, electromagnetic waves may undergo substantial cyclotron damping - particularly the radio waves generated within the magnetosphere of a spinning pulsar. More careful analysis should be made of the escape from the magnetosphere of radiation generated by mechanisms operating in its interior.

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