Abstract:
Models of population of some radiating electron-vibrational states of CO, CN, and C2 molecules are developed. The characteristics of radiation in a chemically nonequilibrium flow behind the front of a strong shock wave in a mixture of gases constituting the Martian atmosphere are calculated. The numerical data are compared with experimental results.
Citation:
V. A. Gorelov, A. Yu. Kireev, S. V. Shilenkov, “Nonequilibrium molecular radiation behind the front of a strong shock wave in the CO2–N2–O2 mixture”, Prikl. Mekh. Tekh. Fiz., 46:2 (2005), 13–22; J. Appl. Mech. Tech. Phys., 46:2 (2005), 160–167