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Generation of pulsar radio emission
Published online by Cambridge University Press: 12 April 2016
Abstract
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