Saha decrements and collisional-radiative recombination and ionization coefficients for a nonequilibrium nitrogen plasma

Statistics – Computation

Scientific paper

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Collisional Plasmas, Nitrogen Plasma, Nonequilibrium Plasmas, Radiative Recombination, Saha Equations, Thermodynamic Equilibrium, Electron Density (Concentration), Electron Energy, Ionization, Optical Thickness, Plasma Radiation, Time Dependence

Scientific paper

Using a time-dependent approach, a collisional-radiative model is developed for a nitrogen plasma. Effective recombination and ionization coefficients are calculated for optically thin and optically thick cases in bound-bound UV radiation. The steady-state population densities for neutral and ionic states are presented in terms of their deviations from Saha equilibrium predictions. These results show the approach of the plasma to local thermodynamic equilibrium as a function of electron temperature and density. The computations focus on temperatures between 1.0 and 3.0 eV and electron densities between 10 to the 16th and 10 to the 19th per cu cm.

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