Two-field models for Rayleigh–Taylor modes are investigated.
The changes due to
external velocity shear (without flow curvature) are reviewed, and the
influences
of the various terms in the models are discussed. It is shown that, in
principle,
velocity shear in combination with dissipation leads to the suppression
of linear
Rayleigh–Taylor modes in the long-time limit. The long-wavelength
modes first
seem to be damped; however, later they show an algebraic growth in time,
before
ultimately the exponential viscous damping wins. In general, the amplitudes
become
very large, and therefore the often-quoted stability of Rayleigh–Taylor
modes
in the presence of velocity shear is more a mathematical artefact than
a real physical
process. Vortices, on the other hand, can lead (together with velocity
shear) to
a quite different dynamical behaviour. Because of a locking of the wave
vectors,
pronounced oscillations appear. This effect is demonstrated by a simple
model
calculation. When vortices and velocity shear are generated from linear
instability, the
resulting oscillatory state finally becomes unstable with respect to Rayleigh–Taylor
modes on a long time scale (‘secondary instability’).