skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Parametric instabilities of damped modes in inhomogeneous plasmas

Technical Report ·
OSTI ID:4326192

Using WKB analysis it is shown that for three-wave backscattering type parametric instabilities in inhomogeneous plasmas no spatial (convective) growth is possible for undamped modes. if one coupled mode is more heavily damped than the other, then spatial growth is possible in both forward and back-scattering. The spatial amplification factor is that obtained by Rosenbluth only if the pump power is sufficiently above a damping-determined threshold but below a threshold for temporal or absolute instability exists for the backscatter instabilities. For the parametric decay instability at omega /sub o/ = 2 omega /sub pe/ in a finite spatial region only a temporal instability is found but no spatial (convective) growth. (auth)

Research Organization:
Colorado Univ., Boulder (USA). Dept. of Astro-Geophysics
DOE Contract Number:
F44620-73-C-0003
NSA Number:
NSA-29-025759
OSTI ID:
4326192
Report Number(s):
AD-763737; CU-1005; AFOSR-TR-73-1134
Resource Relation:
Other Information: Orig. Receipt Date: 30-JUN-74
Country of Publication:
United States
Language:
English

Similar Records

Convective growth of parametrically unstable modes in inhomogeneous media
Journal Article · Sat Jun 01 00:00:00 EDT 1991 · Physics of Fluids B; (USA) · OSTI ID:4326192

Resonant parametric excitations driven by lower-hybrid fields
Journal Article · Sat Nov 01 00:00:00 EST 1980 · Phys. Fluids; (United States) · OSTI ID:4326192

A variational approach to parametric instabilities in inhomogeneous plasmas
Miscellaneous · Fri Dec 31 00:00:00 EST 1993 · OSTI ID:4326192