Dynamic equations for the scalar autocorrelation and scalar-velocity c
ross correlation spectra have been derived for a passive scalar with a
uniform mean gradient using the Eddy Damped Quasi Normal Markovian (E
DQNM) theory. The presence of a mean gradient in the scalar field make
s all correlations involving the scalar axisymmetric with respect to t
he axis pointing in the direction of the mean gradient. Equivalently,
all scalar spectra will be functions of the wave number k and the cosi
ne of the azimuthal angle designated as mu. In spite of this complicat
ion, it is shown that the cross correlation vector can be completely c
haracterized by a single scalar function Q(k). The scalar autocorrelat
ion spectrum, in contrast, has an unknown dependence on mu. However, t
his dependency can be expressed as an infinite sum of Legendre polynom
ials of mu, as first suggested by Herring [Phys. Fluids 17, 859 (1974)
]. Furthermore, since the scalar field is initially zero, terms beyond
the second order of the Legendre expansion are shown to be exactly ze
ro. The energy, scalar autocorrelation, and scalar-velocity cross corr
elation were solved numerically from the EDQNM equations and compared
to results from direct numerical simulations. The results show that th
e EDQNM theory is effective in describing single-point and spectral st
atistics of a passive scalar in the presence of a mean gradient. (C) 1
996 American Institute of Physics.