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Spectroscopic measurements of sub-and supersonic plasma flows for the investigation of atmospheric re-entry shock layer radiation

机译:次和超音速等离子体流的光谱测量,用于研究大气再入激波层辐射

摘要

During planetary atmospheric entries, thermochemical non-equilibrium processes in the shock layer limit the reliability of aerothermal environment prediction. To improve prediction accuracy, non-equilibrium kinetic models are being developed. These models are experimentally assessed through the comparison with well characterized non-equilibrium experiments. For this purpose, the present work is dedicated to the thermodynamic characterization of non-equilibrium in high enthalpy reactive flows. Conversely to common studies that employ short duration facilities to investigate shock layer kinetics, we will assess the possibility of producing significant departure from equilibrium using radio-frequency and microwave stationary plasma flows, including supersonic plasma flows where vibrational non-equilibrium is strongly expected. Suitable spectroscopic diagnostics have been applied allowing future comparisons to be made between the microscopic description of the experiments and theoretical non-equilibrium models.
机译:在行星大气进入过程中,冲击层中的热化学非平衡过程限制了航空热环境预测的可靠性。为了提高预测精度,正在开发非平衡动力学模型。通过与特征明确的非平衡实验进行比较,对这些模型进行了实验评估。为此,本工作致力于高焓反应流中非平衡的热力学表征。与采用短期设施研究冲击层动力学的常规研究相反,我们将评估使用射频和微波固定等离子体流(包括强烈期望振动非平衡的超声等离子体流)产生明显偏离平衡的可能性。已经应用了合适的光谱诊断程序,以便将来可以在实验的微观描述和理论上的非平衡模型之间进行比较。

著录项

  • 作者

    Le Quang Huy Damien;

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  • 年度 2014
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  • 原文格式 PDF
  • 正文语种 en
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