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Aeroheating Testing and Predictions for Project Orion Crew Exploration Vehicle

机译:猎户座项目勘探车的空气加热测试和预测

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An investigation of the aeroheating environment of the Project Orion Crew Exploration Vehicle was performed innthe Arnold Engineering Development Center Hypervelocity Wind Tunnel 9 Mach 8 and Mach 10 nozzles and in thenNASA Langley Research Center 20-Inch Mach 6 Air Tunnel. Heating data were obtained using a thermocoupleinstrumentednu00010:035-scale model [0.1778 m (7 in.) diameter] of the flight vehicle. Runs were performed in thenTunnel 9 Mach 10 nozzle at freestream unit Reynolds numbers of 1 u0002 106 to 20 u0002 106=ft, in the Tunnel 9 Mach 8nnozzle at freestream unit Reynolds numbers of 8 u0002 106 to 48 u0002 106=ft, and in the 20-Inch Mach 6 Air Tunnel atnfreestream unit Reynolds numbers of 1 u0002 106 to 7 u0002 106=ft. In both facilities, enthalpy levels were low and the test gasn(N2 in Tunnel 9 and air in the 20-Inch Mach 6 Air Tunnel) behaved as a perfect gas. These test conditions producednlaminar, transitional, and turbulent data in the Tunnel 9 Mach 10 nozzle; transitional and turbulent data in thenTunnel 9 Mach 8 nozzle; and laminar and transitional data in the 20-Inch Mach 6 Air Tunnel. Laminar and turbulentnpredictions were generated for all wind-tunnel test conditions, and comparisons were performed with thenexperimental data to help define the accuracy of the computational method. In general, it was found that bothnlaminar data and predictions and turbulent data and predictions agreed to within less than the estimated u000312%nexperimental uncertainty estimate. Laminar heating distributions from all three data sets were shown to correlatenwell and demonstrated Reynolds numbers independence when expressed in terms of the Stanton number based onnadiabatic-wall-recovery enthalpy. Transition-onset locations on the lee-side centerline were determined from thendata and correlated in terms of boundary-layer parameters. Finally, turbulent heating augmentation ratios werendetermined for several body-point locations and correlated in terms of the boundary-layer momentum Reynoldsnnumber.
机译:在Arnold工程开发中心超高速风洞9 Mach 8和Mach 10喷嘴以及随后的NASA Langley研究中心20英寸Mach 6空气隧道中,对“猎户座”乘员探索车的空气加热环境进行了调查。使用飞行器的热电偶仪表nu00010:035比例模型[直径0.1778 m(7英寸)]获得加热数据。然后在9号马赫10喷嘴的自由流单位雷诺数为1 u0002 106到20 u0002 106 = ft的通道中,在9号马赫8喷嘴的自由流单位雷诺数为8 u0002 106到48 u0002 106 = ft处,并在20英寸马赫6空气隧道atnfreestream单位雷诺数1 u0002 106至7 u0002 106 = ft。在这两个工厂中,焓值都很低,并且测试气体(隧道9中的N2和20英寸马赫6空气隧道中的空气)表现为理想气体。这些测试条件在Tunnel 9 Mach 10喷嘴中产生层流,过渡和湍流数据;然后在隧道9马赫8喷嘴中获得过渡和湍流数据;和20英寸6马赫空气隧道的层流和过渡数据。针对所有风洞测试条件生成了层流和湍流预测,并与随后的实验数据进行了比较,以帮助定义计算方法的准确性。通常,发现层流数据和预测以及湍流数据和预测都在小于估计的不确定性估计的范围内达成一致。当根据基于绝热壁回收焓的斯坦顿数表示时,来自所有三个数据集的层流加热分布显示出相关性,并证明了雷诺数的独立性。根据当时的数据确定背风侧中心线上的过渡开始位置,并根据边界层参数进行关联。最后,确定了几个体点位置的湍流加热增加率,并根据边界层动量雷诺数进行了相关。

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