A simple model of Bernstein mode parametric excitation near the electr
on plasma frequency in a subcritical laser-produced plasma is presente
d. It is argued that the instability threshold of such modes might bec
ome much lower than the usual thresholds for both convective and absol
ute Raman scattering, in particular, near the so-called ''omega(qn)''
resonances. This would occur in high-temperature plasmas (2-5 keV) and
over very small (about ten microns long) regions of flat magnetic fie
ld and plasma density, corresponding to hot spot locations. A special
emphasis is placed on a simplified formulation of the growth rates and
thresholds for parameters domains wherein Bernstein mode parametric e
xcitation might be of importance, to allow applications in any experim
ental situation. Many features of the resulting backscatter compare fa
vorably with experimental observations. (C) 1997 American Institute of
Physics.