Turbulent equipartition is investigated for the nonlinear evolution of
pressure driven flute modes of a plasma in an inhomogeneous magnetic
field. The Rayleigh-Taylor instability is recovered by linear stabilit
y analysis, and occurs when the pressure profile is more peaked than t
he profile of the magnetic field. Numerical solutions of the model equ
ations on a bounded domain with sources and sinks show that the flux-d
riven turbulent fluctuations give rise to up-gradient transport, a ''p
inch flux,'' of heat or particles. The averaged equilibrium density an
d temperature profiles approach n similar to B and T similar to B-2/3,
as predicted by turbulent equipartition.