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Non- Equilibrium Radiation and Physical- Chemical Processes in Martian Atmosphere in Strong Shock Waves

机译：强冲击波中火星大气的非平衡辐射与物理化学过程

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《AIAA Aerospace Sciences Meeting and Exhibit》|2005年|P.1-6|共6页
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E. Anokhin; A. Starikovskii;
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中图分类航空;
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1. Measurements of non-equilibrium and equilibrium temperature behind a strong shock wave in simulated martian atmosphere [J] . Xin Lin, Xi-Long Yu, Fei Li, 力学学报：英文版 . 2012,第005期

机译：模拟火星大气中强冲击波背后的非平衡和平衡温度的测量
2. Numerical Investigation of a Model of Nonequilibrium Radiation behind a Shock Front in the Martian Atmosphere [J] . A. S. Dikalyuk, S. T. Surzhikov Fluid Dynamics . 2013,第1期

机译：火星大气激波锋后非平衡辐射模型的数值研究
3. Radiation of Ultra Low Frequency Electromagnetic Waves from Atmosphere under the Influence of Strong Shock Waves [J] . A.R.Aramyan, S.A.Aramyan, S.G.Bilén, 中国物理快报：英文版 . 2015,第003期

机译：强冲击波影响下大气中超低频电磁波的辐射
4. Non- Equilibrium Radiation and Physical- Chemical Processes in Martian Atmosphere in Strong Shock Waves [C] . American Institute of Aeronautics and Astronautics Aerospace Sciences Meeting and Exhibit . 2005

机译：强震波浪中火星氛围中的非平衡辐射和物理化学过程
5. TVD flux-difference split methods for high-speed thermochemical nonequilibrium flows with strong shocks. [D] . Groth, Clinton P. T. 1993

机译：TVD磁通差分流方法可用于具有强烈冲击的高速热化学非平衡流。
6. On the strong and selective isotope effect in the UV excitation of N2 with implications toward the nebula and Martian atmosphere [O] . B. H. Muskatel, F. Remacle, Mark H. Thiemens, 2011

机译：关于N2的紫外线激发中的强选择性同位素效应对星云和火星大气有影响
7. A Shock Tube Study on Nonequilibrium Radiation of Strong Shock Waves in Low-Density Air. [O] . Hiroki HONMA, Toshihiro MORIOKA, Nariaki SAKURAI, 1998

机译：低密度空气强冲击波非醌辐射的冲击管研究。
8. Study of Optical Radiation in the Wavelength Regions of 0.4216 mu, 0.4278 mu, 0.4835 mu, and 0.5165 mu Behind Normal Shock Waves in a Simulated Martian Atmosphere [R] . Arnold, J. O., Dyner, H. B., Modica, A. P., 1968

机译：模拟火星大气层正常冲击波波长区域的光辐射研究0.4216亩，0.4278亩，0.4835亩和0.5165亩

Non- Equilibrium Radiation and Physical- Chemical Processes in Martian Atmosphere in Strong Shock Waves

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