Abstract
The results of measuring the radiation characteristics of the shock-heated mixture of CO2–N2 simulating the atmosphere of Mars are presented. Experiments carried out on a modified double-diaphragm shock tube (DDST-M) of the Institute of Mechanics, Moscow State University for two combinations of initial pressures and velocities of the shock wave: 5.4–6.8 km/s at a pressure of 1.0 Torr and 5.3–8.1 km/s at a pressure of 0.3 Torr. Panoramic radiation spectra in the wavelength range of 200 to 850 nm (ultraviolet and visible spectral ranges) and the temporal dependence of the radiation intensity of one of the most intense emission bands were obtained. The measurement data are compared with the experimental data of other authors.
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Funding
This study was supported by the Russian Foundation for Basic Research, grant no. 20-08-00343, and as part of a state assignment of the Ministry of Science and Higher Education of the Russian Federation “Experimental and theoretical study of kinetic processes in gases” (state registration number AAAA-A19-119012990112-4).
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Kozlov, P.V., Zabelinsky, I.E., Bykova, N.G. et al. Experimental Study of the Radiation Characteristics of a CO2–N2 Mixture Behind the Front of a Strong Shock Wave. Russ. J. Phys. Chem. B 15, 989–994 (2021). https://doi.org/10.1134/S1990793121060208
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DOI: https://doi.org/10.1134/S1990793121060208