  Recent work has shown that ions are strongly coupled in atmospheric pressure
plasmas when the ionization fraction is sufficiently large, leading to a
temperature increase from disorder-induced heating that is not accounted for in
standard modelling techniques. Here, we extend this study to molecular plasmas.
A main finding is that the energy gained by ions in disorder-induced heating
gets spread over both translational and rotational degrees of freedom on a
nanosecond timescale, causing the final ion and neutral gas temperatures to be
lower in the molecular case than in the atomic case. A model is developed for
the equilibrium temperature that agrees well with molecular dynamics
simulations. The model and simulations are also applied to pressures up to ten
atmospheres. We conclude that disorder-induced heating is a significant and
predictable phenomenon in molecular atmospheric pressure plasmas.
