“…This model consists in writing a continuity equation for the population of each vibrational level of molecules, determining species densities and their internal distributions [2], including not only vibrational states, but also electronically excited states [3] as well as non-maxwellian electron energy distribution functions (EEDF) by solving an adequate Boltzmann equation [4,5]. With few exceptions (see [6,7,8]), applications of the STS approach to high enthalpy flow simulation have been very limited, due to the significant computing time required to conduct even 1-D simulations [9,10,11].…”