The stability properties of an ideal magnetohydrodynamic (MHD) fluid (
compressible) in an arbitrary state of motion is explored. A stability
condition is formulated in general terms based on the concept of a Ly
apunov functional for the system which can be taken to be the Hamilton
ian. Special consideration is given to stationary systems where the fl
uid is bounded by a surface on which the normal component of the fluid
velocity is zero. For this case a necessary and sufficient condition
for stability in terms of an energy principle is formulated. This can
be considered to be a generalization of the classic MHD energy princip
le. A comparison to normal mode solutions is made. Systems being subje
cted to forced oscillations around a static equilibrium that may be un
stable are of prime interest for dynamic stabilization problems. The p
resent theory also includes results relevant to this type of system, a
lthough no details of such problems are presented. The emphasis is on
general theory, however, one example of an ordinary fluid which is rot
ating is discussed in order to get a better understanding of the theor
etical results. (C) 1997 American Institute of Physics.