A closure for the compressible portion of the pressure-strain covariance is
developed. It is shown that, within the context of a pressure-strain closu
re assumption linear in the Reynolds stresses, an expression for the pressu
re-dilatation can be used to construct a representation for the pressure-st
rain. Additional closures for the unclosed terms in the Favre-Reynolds stre
ss equations involving the mean acceleration are also constructed. The clos
ures accommodate compressibility corrections depending on the magnitude of
the turbulent Mach number, the mean density gradient, the mean pressure gra
dient, the mean dilatation, and, of course, the mean velocity gradients. Th
e effects of the compressibility corrections on the Favre-Reynolds stresses
are consistent with current DNS results. Using the compressible pressure-s
train and mean acceleration closures in the Favre-Reynolds stress equations
an algebraic closure for the Favre-Reynolds stresses is constructed. Notew
orthy is the fact that, in the absence of mean velocity gradients, the mean
density gradient produces Favre-Reynolds stresses in accelerating mean flo
ws. Computations of the mixing layer using the compressible closures develo
ped are described. Favre-Reynolds stress closure and two-equation algebraic
models are compared to laboratory data for the mixing layer. Experimental
data from diverse laboratories for the Favre-Reynolds stresses appears inco
nsistent and, as a consequence, comparison of the Reynolds stress predictio
ns to the data is not conclusive. Reductions of the kinetic energy and the
spread rate are consistent with the sizable decreases seen in these classes
of flows. (C) 1999 American Institute of Physics. [S1070-6631(99)00809-0].