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Analytical results on the breakdown of the convective amplifier model caused by space–time random fluctuations (1995)

Mounaix, Philippe

[S.l.] : American Institute of Physics (AIP)

Physics of Plasmas 2 (1995), S. 1804-1806

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ISSN: 1089-7674

Source: AIP Digital Archive

Topics: Physics

Notes: The space and time behavior of backscattering instabilities is computed analytically in the strongly damped regime and in the presence of space–time random fluctuations. The fluctuations are described by a Gaussian process with exponentially decaying correlation function. The breakdown of the strongly damped model of the instability is obtained as a divergence of the average amplitude and intensity of the backscattered light [H. A. Rose and D. F. DuBois, Phys. Rev. Lett. 72, 2883 (1994)]. The length and time it takes for this divergence to occur is analytically computed. © 1995 American Institute of Physics.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1063/1.871333

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