The potential for laser-plasma instability is a serious concern for in
direct-drive inertial confinement fusion (ICF), where laser beams illu
minate the interior of a cavity (called a hohlraum) to produce x-rays
for imploding a fusion capsule symmetrically. The speckled nature of l
aser beams used in ICF is an important factor in laser-plasma instabil
ity processes. For example, models which calculate the spatial growth
of convective instability by properly accounting for the laser speckle
s successfully predict the observed onsets of backscattering due to st
imulated Brillouin and Raman scattering instabilities (SBS and SRS). A
ssuming pump depletion as the only saturation mechanism in these model
s results in very large predicted levels of SBS and SRS backscattering
from the long-scale plasmas expected in ignition hohlraums. However,
in the long-scale plasmas studied in the Nova and Trident lasers [E. M
. Campbell, Rev. Sci. Instrum. 57, 2101 (1986) and N. K. Moncur et al.
, Appl. Opt. 34, 4274 (1995)], SRS and SBS are observed to saturate mu
ch below the levels expected from pump depletion. While the mechanism
of SBS saturation is not understood at present, the observations of SR
S saturation are qualitatively understood. (C) 1997 American Institute
of Physics.