Premixed methane combustion in a partially stirred reactor (PaSR) is s
tudied numerically. The effects of turbulent stirring rate on NO, CO,
and other quantities are computed. The chemistry is represented by a '
'full'' scheme (27 species, 77 reactions) in the baseline study. Turbu
lence is accounted for by the ''IEM'' (Interaction-by-Exchange-with-th
e-Mean) submodel. The PaSR is described by a system of (N(s) + 1) x N(
p) first-order coupled o.d.e.'s in time, where N(s) = number of specie
s, and N(p) = number of particles. The model is well suited to paralle
l computers, without which the present study would not have been pract
ical. The speedup over serial computers is essentially linear in the n
umber of processors used, until the number of particles per processor
becomes small enough (< 10) to affect load balance. The conditions are
30 atm, 1200-K inlet temperature, 800-K equilibrium temperature rise,
and 2-ms reactor residence time (in the PSR limit). In the PFR limit
the flow just starts to ignite, while in the PSR limit temperatures ar
e very near equilibrium. PaSR simulations are conducted in the range 1
00-5000 Hz (mixing frequency), and in each case converge to a stochast
ic steady state and span the PFR-PSR limits smoothly. The correlation
of NO with particle age decreases as frequency increases, and is withi
n expected limits. The OH levels are uniform to within a factor of two
in this frequency range, which is consistent with the ''distributed''
OH structures observed in turbulent diffusion flames. Simulations wit
h a 25-step ''skeletal'' scheme agreed well with the baseline study ab
ove 1,000 Hz, but are about 400 K low on mean temperature at 100 Hz. T
he corresponding four-step ''reduced'' scheme failed to ignite in all
cases, suggesting a need for reduced schemes which do not assume that
the radicals are in a chemically steady state.