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Computational and experimental investigation of two-dimensional scramjet inlets and hypersonic flow over a sharp flat plate.

机译:二维超燃冲压进气口和尖锐​​平板上的高超音速流动的计算和实验研究。

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The WIND code was employed to compute the hypersonic flow in the shock wave boundary layer merged region near the leading edge of a sharp flat plate. Solutions were obtained at Mach numbers from 9.86 to 15.0 and free stream Reynolds numbers of 3,467 to 346,700 in−1 (1.365 · 105 to 1.365 · 107 m−1) for perfect gas conditions. The numerical results indicated a merged shock wave and viscous layer near the leading edge. The merged region grew in size with increasing free stream Mach number, proportional to M 2/Re. Profiles of the static pressure in the merged region indicated a strong normal pressure gradient (∂p/∂y). The normal pressure gradient has been neglected in previous analyses which used the boundary layer equations.; The shock wave near the leading edge was thick, as has been experimentally observed. Computed shock wave locations and surface pressures agreed well within experimental error for values of the rarefaction parameter, χ/M2 0.3. A preliminary analysis using kinetic theory indicated that rarefied flow effects became important above this value. In particular, the WIND solution agreed well in the transition region between the merged flow, which was predicted well by the theory of Li and Nagamatsu, and the downstream region where the strong interaction theory applied.; Additional computations with the NPARC code, WIND's predecessor, demonstrated the ability of the code to compute hypersonic inlet flows at free stream Mach numbers up to 20. Good qualitative agreement with measured pressure data indicated that the code captured the important physical features of the shock wave - boundary layer interactions. The computed surface and pitot pressures fell within the combined experimental and numerical error bounds for most points. The calculations demonstrated the need for extremely fine grids when computing hypersonic interaction flows.
机译:WIND代码用于计算尖锐平板前缘附近的冲击波边界层合并区域中的高超音速流。在 -1 (1.365·10 5 到1.365·10 7 <的自由度下,以马赫数从9.86到15.0和自由流雷诺数从3,467到346,700获得溶液。 / super> m −1 )以达到理想的气体条件。数值结果表明在前缘附近有合并的冲击波和粘性层。合并区域的大小随自由流马赫数的增加而增加,与M 2 / Re 成正比。合并区域中的静压力曲线表明有很强的法向压力梯度(∂p/∂y)。在以前的使用边界层方程的分析中,忽略了法向压力梯度。正如实验观察到的那样,前缘附近的冲击波很厚。计算的冲击波位置和表面压力在稀疏参数χ/ M 2 <0.3的实验误差范围内吻合得很好。使用动力学理论进行的初步分析表明,稀疏流动效应在此值以上变得很重要。尤其是,WIND解在Li和Nagamatsu的理论所预测的合并流与应用强相互作用理论的下游区域之间的过渡区域中非常吻合。 WIND的前身NPARC代码的其他计算证明了该代码在自由流马赫数高达20的情况下计算超音速入口流量的能力。与测量压力数据的良好定性表明,该代码捕获了冲击波的重要物理特征。 -边界层相互作用。对于大多数点,计算得到的表面和皮托管压力都落在组合的实验和数值误差范围内。计算结果表明,在计算高超声速相互作用流时需要极细的网格。

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