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Electron beam radiation by collective Compton boosting of strong turbulence
Several strong relativistic beam–plasma experiments have found powerful broadband microwave emission far above the plasma line. To model these experiments, consider scattering of electrons by cavitons of plasma turbulence of size D. This yields radiation Compton boosted to frequencies ∼2γ2 c/D and r...
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Published in: | Physics of fluids. B, Plasma physics Plasma physics, 1992-12, Vol.4 (12), p.4111-4120 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Several strong relativistic beam–plasma experiments have found powerful broadband microwave emission far above the plasma line. To model these experiments, consider scattering of electrons by cavitons of plasma turbulence of size D. This yields radiation Compton boosted to frequencies ∼2γ2
c/D and relativistically beamed. To attain the observed powers (up to 108 W) the beam must be bunched. Several models for beam density fluctuation statistics can give the observed power, but only broad distributions, such as a Gaussian electrostatic spectrum in k, can yield a qualitatively wide radiation spectrum. Power scalings can be checked in future experiments. |
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ISSN: | 0899-8221 2163-503X |
DOI: | 10.1063/1.860318 |