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Experimental and Numerical Investigation of Air Radiation in Superorbital Expanding Flow

机译:超轨道膨胀流中空气辐射的实验与数值研究

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To investigate air radiation in expanding flows and provide experimental data for validating associated computational models, experiments were conducted in the X2 expansion tunnel facility at the Centre for Hypersonics of the University of Queensland. A 54° turning angle wedge model was employed to generate steady expanding flows with inflow total enthalpies of 50.7, 63.4 and 75.4 MJ/kg. VUV spectra from 118 to 180 nm were acquired across the wedge at three equispaced distances away from the top of the model, as well as through its top surface. High speed filtered images were also obtained by coupling a Shimadzu 1 MHz high speed camera to a bandpass filter to obtain calibrated images of the 777 nm oxygen triplet. Both the across-wedge VUV spectra and filtered images of the 777 nm atomic oxygen were compared with NEQAIR simulations, which were performed using flow field data from two-dimensional CFD simulations with two-temperature 11-species air chemistry utilising the in-house Navier-Stokes flow solver Eilmer3.
机译:为了研究膨胀流中的空气辐射并为验证相关的计算模型提供实验数据,在昆士兰大学高超音速中心的X2膨胀隧道设施中进行了实验。使用54°转角楔形模型生成稳定的膨胀流,流入总焓为50.7、63.4和75.4 MJ / kg。横跨楔形,在距模型顶部三个距离以及顶部表面的三个等距距离处,获取了118至180 nm的VUV光谱。通过将Shimadzu 1 MHz高速相机与带通滤光片耦合以获得777 nm氧气三重态的校准图像,也可以获得高速滤波图像。楔形VUV光谱和777 nm原子氧的过滤图像都与NEQAIR模拟进行了比较,NEQAIR模拟是使用二维CFD模拟的流场数据与内部使用的Navier进行的两温度11种空气化学反应进行的-斯托克斯流量求解器Eilmer3。

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