The behaviour of internal gravity wave packets approaching a critical
level is investigated through numerical simulation. Initial-value prob
lems are formulated for both small- and large-amplitude wave packets.
Wave propagation and the early stages of interaction with the mean she
ar are two-dimensional and result in the trapping of wave energy near
a critical level. The subsequent dynamics of wave instability, however
, are fundamentally different for two- and three-dimensional calculati
ons. Three-dimensionality develops by transverse convective instabilit
y of the two-dimensional wave. The initially two-dimensional flow even
tually collapses into quasi-horizontal vortical structures. A detailed
energy balance is presented. Of the initial wave energy, roughly one
third reflects, one third results in mean flow acceleration and the re
mainder cascades to small scales where it is dissipated. The detailed
budget depends on the wave amplitude, the amount of wave reflection be
ing particularly sensitive.