SIMULTANEOUS EXCITATION OF PARAMETRIC DECAY CASCADES AND OF THE OSCILLATING 2-STREAM INSTABILITY IN ONE-DIMENSIONAL NUMERICAL SIMULATIONS BASED ON ZAKHAROV EQUATIONS
Ra. Sprague et Ja. Fejer, SIMULTANEOUS EXCITATION OF PARAMETRIC DECAY CASCADES AND OF THE OSCILLATING 2-STREAM INSTABILITY IN ONE-DIMENSIONAL NUMERICAL SIMULATIONS BASED ON ZAKHAROV EQUATIONS, J GEO R-S P, 100(A12), 1995, pp. 23959-23972
The excitation of a parametric decay cascade and of the oscillating tw
o-stream instability (OTSI) have been predicted earlier by one-dimensi
onal and two-dimensional weak turbulence approximations for observatio
ns with the 430-MHz radar for ionospheric modification experiments at
Arecibo, for heights 1-2 km below the reflection height of the pump wa
ve. For the same height range the present numerical simulations, using
a version of the one-dimensional driven and damped Zakharov system of
equations, are shown to lead over a limited range of pump powers to t
he simultaneous excitation of a weak turbulence decay cascade and of t
he OTSI or modulational instability. The linearized form of the Zakhar
ov equations is used to derive the functional dependence of the transf
er of power from one Langmuir wave to another on the parameters of the
two waves, Comparison of that function with the more correct version
derived from kinetic theory was then used to guide the choice of the d
amping coefficient of ion acoustic waves, With that choice the simulat
ions show that for a pump power that exceeds the threshold for excitat
ion of the parametric decay instability by a factor less than about 3,
the OTSI is not excited in the steady state which only shows the exci
tation of the parametric decay cascade, For pump powers that exceed th
e threshold power by a factor greater than about 3 but are not great e
nough to lead to a Langmuir condensate and ultimately to strong cavita
tional Langmuir turbulence, the simulations show the simultaneous exci
tation of a weak turbulence cascade and of the OTSI, These conclusions
agree qualitatively with the conclusions reached on the basis of earl
ier weak turbulence approximations.