In the investigation of hypersonic rarefied flows, it is important to
consider the effects of thermal nonequilibrium on the dissociation rat
es. Because the vibrational mode requires a finite time to relax, vibr
ational energy may not be available for dissociation immediately behin
d the shock. In this way, the dissociation of the preshock species can
be delayed for a significant portion of the hypersonic shock layer. T
he majority of implementations of the direct simulation Monte Carlo (D
SMC) method of Bird do not account for vibration-dissociation coupling
. Haas and Boyd have proposed the vibrationally favored dissociation (
VFD) model to accomplish this task. Their model made use of measuremen
ts of induction distance to determine model constants. A more general
expression has been derived that does not require any experimental inp
ut. The model is used to calculate one-dimensional shock waves in nitr
ogen and the flow past a lunar transfer vehicle (1,TV). For the condit
ions considered in the simulation, the influence of vibration-dissocia
tion coupling on heat transfer in the stagnation region of the LTV can
be important.