Direct numerical simulation (DNS) is used to examine scalar correlatio
n in low Mach number, polytropic, homogeneous, two-dimensional turbule
nce (M(s) less than or equal to 0.7) for which the initial conditions,
Reynolds, and Mach numbers have been chosen to produce three types of
flow suggested by theory: (a) nearly incompressible flow dominated by
vorticity, (b) nearly pure acoustic turbulence dominated by compressi
on, and (c) nearly statistical equipartition of vorticity and compress
ions. Turbulent flows typical of each of these cases have been generat
ed and a passive scalar field imbedded in them. The results show that
a finite-difference based computer program is capable of producing res
ults that are in reasonable agreement with pseudospectral calculations
. Scalar correlations have been calculated from the DNS results and th
e relative magnitudes of terms in low-order scalar moment equations de
termined. It is shown that the scalar equation terms. with explicit co
mpressibility are negligible on a long time-averaged basis, A physical
-space EDQNM model has been adapted to provide another estimate of sca
lar correlation evolution in these same two-dimensional, compressible
cases. The use of the solenoidal component of turbulence energy, rathe
r than total turbulence energy, in the EDQNM model gives results close
r to those from DNS in all cases. (C) 1995 American Institute of Physi
cs.