caa a22 4500 469100230 CHVBK 20180323133042.0 cr unu---uuuuu 170328e19920101xx s 000 0 eng 10.1007/BF01054183 doi (NATIONALLICENCE)springer-10.1007/BF01054183 Emission and radiative cooling of xenon plasma behind a strong shock front [Elektronische Daten] [S. Makarychev, G. Smekhov, M. Yalovik] A numerical and experimental investigation of the emissivity and radiative cooling of xenon plasma in strong shock waves with Mach numbers M=16-45, including experimentally up to M=28, has been made. It is shown that under these conditions the equilibrium temperature behind the shock wave can be reduced by cooling by 1.5-2 times. Plenum Publishing Corporation, 1992 Makarychev S. Moscow aut Smekhov G. Moscow aut Yalovik M. Moscow aut Fluid Dynamics Kluwer Academic Publishers-Plenum Publishers 27/1(1992-01-01), 116-121 0015-4628 27:1<116 1992 27 10697 https://doi.org/10.1007/BF01054183 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/BF01054183 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Makarychev S. Moscow aut NATIONALLICENCE 700 1- Smekhov G. Moscow aut NATIONALLICENCE 700 1- Yalovik M. Moscow aut NATIONALLICENCE 773 0- Fluid Dynamics Kluwer Academic Publishers-Plenum Publishers 27/1(1992-01-01), 116-121 0015-4628 27:1<116 1992 27 10697 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer