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Effect of Heavy-Particle Impact Excitation Processes on Post Shock Nonequilibrium Air radiation
Conference paper   Peer reviewed

Effect of Heavy-Particle Impact Excitation Processes on Post Shock Nonequilibrium Air radiation

A Lemal, Carolyn Jacobs, M Y Perrin, C O Laux, P Tran and E Raynaud
Proceedings of the 8th European Symposium on Aerothermodynamics for Space Vehicles, pp.1-10
European Symposium on Aerothermodynamics for Space Vehicles, 8th (Lisbon, Portugal, 02-Mar-2015–06-Mar-2015)
European Space Agency
2015
url
http://esaconferencebureau.com/Custom/15A01/Papers/Room%201.1/Tuesday/Measurement%20techniques%20II/86325_Lemal.pdfView
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Abstract

Aerospace Engineering heavy-particle impact collisional-radiative (CR) model Ecole Centrale Paris vacuum ultra violet (VUV) infrared (IR) spectral ranges spectral ranges
The absolute radiation measurements obtained in the Electric-Arc driven Shock-Tube (EAST) facility at NASA Ames Research Center were analyzed to test the collisional-radiative (CR) model developed at Ecole Centrale Paris. Two conditions representative of Earth reentry at 10.54 and 11.17 km/s were investigated in the vacuum ultra violet (VUV) and infrared (IR) spectral ranges. For each of the conditions, the corresponding CCD images were analyzed. The electron number density was inferred from Starkbroadened nitrogen and Hα lines. Comparisons with the predicted electron number density profiles enabled us to validate the ionization rate constant model implemented in the flowfield. For both freestream conditions and all the spectral ranges, the predictions of the initial intensity rises are improved when the total spatial smearing (due to the shock motion, the optics and the camera) is taken into account. The nonequilibrium intensities observed in the VUV and IR spectral ranges were underpredicted by the CR model when only electron-impact excitation and ionization processes were taken into account. Then, the effect of heavy-particle impact processes was studied by applying various heavy-particle impact excitation models. The nonequilibrium peak intensities observed in the VUV and IR spectral ranges were shown to be controlled by heavy-particle impact excitation processes.

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