Spectroscopic Analysis of Nonequilibrium Excited State Chemistry in a NASA Arc Jet

Abstract

To support the determination of total specific enthalpy of the plasma flow of the 60 MW Interaction Heating Facility at NASA Ames Research Center, spectroscopic measurements of nonequilibrium emission were performed in the freestream. In the visible to near-infrared wavelength region, the most prominent emission was from molecular , and in the ultraviolet region, the spectra were dominated by emission from molecular NO. The only atomic lines observed were those of copper (an erosion product of the electrodes). The bands of the First Positive System of () differed significantly from spectra computed assuming only thermal excitation, suggesting overpopulation of the high vibrational states of the B state of . Populations of these high vibrational levels (peaking at ) of the B state were determined by scaling spectra simulated for each upper vibrational state separately. The overpopulation of the high vibrational levels is assigned to inverse predissociation of neutral atoms into the B state at via level-crossing processes with the state. The and 13 emission has been used to determine N atom densities, which agree very well between the different experiment campaigns and with the computational-fluid-dynamics simulation of these flows.