  The propagation of compressional MHD waves is studied for an externally
driven system. It is assumed that the combined action of the external sources
and sinks of the entropy results in the harmonic oscillation of the entropy
(and temperature) in the system. It is found that with the appropriate resonant
conditions fast and slow waves get amplified due to the phenomenon of
parametric resonance. Besides, it is shown that the considered waves are
mutually coupled as a consequence of the nonequilibrium state of the background
medium. The coupling is strongest when the plasma $\beta \approx 1$. The
proposed formalism is sufficiently general and can be applied for many
dynamical systems, both under terrestrial and astrophysical conditions.
