A popular contemporary approach in predicting enhanced flame speeds in
premixed turbulent combustion involves averaging or closure theories
for the G-equation involving both large-scale flows and small-scale tu
rbulence. The G-equation is a Hamilton-Jacobi equation involving advec
tion by an incompressible velocity field and nonlinear dependence on t
he laminar flame speed; this G-equation has been derived from the comp
lete Navier-Stokes equations under the tacit assumptions that the velo
city field varies on only the integral stale and that the ratio of the
flame thickness to this integral scale is small. Thus there is a pote
ntial source of error in using the averaged G-equation with turbulent
velocities varying on length scales smaller than the integral scale in
predicting enhanced flame speeds. Here these issues are discussed in
the simplest context involving velocity fields varying on two scales w
here a complete theory of nonlinear averaging for predicting enhanced
flame speeds without any nd hoc approximations has been developed rece
ntly by the authors. The predictions for enhanced flame speeds of this
complete averaging theory versus the averaging approach utilizing the
G-equation are compared here in the simplest context involving a cons
tant mean flow and a small-scale steady periodic flow where both theor
ies can be solved exactly through analytical formulas. The results of
this comparison are summarized briefly as follows: The predictions of
enhanced flame speeds through the averaged G-equation always underesti
mate those computed by complete averaging. Nevertheless, when the tran
sverse component of the mean flow relative to the shear is less than o
ne in magnitude, the agreement between the two approaches is excellent
. However, when the transverse component of the mean flow relative to
the shear exceeds one in magnitude, the predictions of the enhanced fl
ame speed by the averaged G-equation significantly underestimate those
computed through complete nonlinear averaging, and in some cases, by
more than an order of magnitude. (C) 1995 American Institute of Physic
s.