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Generation of pulsar radio emission

Published online by Cambridge University Press:  12 April 2016

Yu.E. Lyubarskii
Yu.E. Lyubarskii*
Affiliation:
Institute of Radio Astronomy, Krasnoznamyonnaya St.4, 310002, Kharkov, Ukraine

Abstract

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The generation of radio emission from plasma waves excited by two-stream instability in pulsar magnetospheres is considered. Induced scattering transforms the excited longitudinal waves into waves that escape freely in the form of transverse electromagnetic waves. It is shown that the spectrum and the luminosity of the generated radio emission are compatible with those observed.

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 387 - 388
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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