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Convective Brillouin amplification in drifting plasmas

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.863617· OSTI ID:5874467
Previous work on the absolute instability of Brillouin scatter in drifting plasmas is extended to the case of convective amplification. It is found that, similar to temporal growth rates for the absolute instability, forward oblique scatter has the highest spatial gain, with backscatter near a minimum. To agree with experimental results on outward scattered light, source terms are required which must be many orders of magnitude above thermal. Although in the heavy ion damping regime self-limiting via ion heating decreases the sensitivity of the final reflectivity to the source strength, there is no evidence of a scattering limit when pump depletion is small (the normal experimental situation).
Research Organization:
INRS-Energie, Varennes, Quebec, Canada J0L 2P0
OSTI ID:
5874467
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 25:1; ISSN PFLDA
Country of Publication:
United States
Language:
English