Third and higher harmonic plasma emission due to Raman scattering

Details Third and higher harmonic plasma emission due to Raman scattering Third and higher harmonic plasma emission due to Raman scattering

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jplph..38..199c&link_type=abstract

Journal of Plasma Physics (ISSN 0022-3778), vol. 38, Oct. 1987, p. 199-208.

Physics

Plasma Physics

10

Harmonic Radiation, Plasma Radiation, Plasma Turbulence, Plasma Waves, Raman Spectra, Electrostatic Waves, Magnetohydrodynamic Stability, Transverse Waves, Wave Interaction

Scientific paper

The theory for third and higher harmonic plasma emission by the weak turbulence (or random phase) process L + T prime to T (where L denotes a Langmuir wave, and T and T prime denote transverse waves) is developed. Kinematic constraints on the characteristics and growth lengths of waves participating in the wave processes are identified. The cases of L waves produced either directly by a streaming instability, or by the decay L to L prime + S (S is an ion sound wave) of L waves generated by a streaming instability, are considered. Limits on the brightness temperature of the radiation are determined, and expressions for the growth rate and path-integrated wave temperatures are derived.

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