喷管内二次喷射的激波测量与分析

研究了不同喷射位置、喷射马赫数和喷射角度的气体二次喷射混合流场的弓形激波形状。在二维矩形喷管内进行二次喷射试验,用纹影仪拍摄得到激波照片。将由照片换算得到了激波半径与用爆炸理论计算的结果相比较,证明爆炸波解在计算激波半径方面提供了与实验较符合的结果。     

月球探测器软着陆机构着陆腿模型与仿真分析

给出了着陆动力学分析的数学模型,并在分析铝蜂窝材料缓冲特性的基础上,建立了 铝蜂窝缓冲器模型,将其应用于软着陆机构单条着陆腿冲击仿真。仿真结果表明,该模型在 缓冲行程、能量吸收及缓冲后加速度响应峰值等方面与试验结果基本一致。为软着陆机构着 陆冲击动力学分析时铝蜂窝建模提供参考。     

温敏漆技术及其在边界层转捩测量中的应用

A temperature sensitive paint (TSP) technique is developed for the request of boundary layer transition measurement, and a test of hypersonic boundary layer measurement of a flat plate is done in CARDC 0.6m shock tunnel. By use of the TSP technique, the measurement of the hypersonic boundary layer transition of slab has been done in the shock tunnel. The test nominal Mach numbers are 8 and 10, the unit Reynolds numbers are 2.45×10 7/m and 4.48× 10 6/m respectively, and the yaw angle is 20°. The data of heat transfer and transition position obtained by the TSP and measurement results of the thin film heat transfer sensor match well. The results illustrate that the TSP technique has the ability to measure the hypersonic boundary layer transition of simple model qualitatively and quantitatively in shock tunnel.     

飞行器结构部件冲击响应谱（SRS）匹配技术研究

本文介绍了利用ＴＭＳ３２０Ｃ３０高速数据处理芯片构成ＳＲＳ分析与匹配系统的配置方案，以及利用此系统的特定子波加权合成－冲击波形，并反复修正此冲击波形，使其所产生的ＳＲＳ与规定的谱值相匹配的迭代技术。     

导叶间隙不确定性对可调向心涡轮影响数值研究

为了评估可调向心涡轮导流叶片叶顶及叶根间隙尺寸不确定性对涡轮级性能的影响,首先将喷嘴环叶片大开度模型的单通道定常数值结果与实验数据对比;然后以导流叶片小开度涡轮为研究对象,数值模拟导叶两端叶顶间隙尺寸多种分配模型三维流场,总结出导叶间隙不确定性与涡轮级性能之间相应变化规律;最后选取导叶两端间隙平均分配模型和最优涡轮性能下间隙分配模型开展多通道定常/非定常计算,用于分析间隙分配变化对转静干涉影响。研究结果表明:当导流叶片轮缘侧间隙尺寸占全部间隙尺寸5%~15%范围时,涡轮级效率较高;当导叶间隙全部集中在轮缘侧时,涡轮效率较低;最高、最低效率差别约为6%。间隙泄漏流变化将引起下游转子叶片进口气流角发生变化,进而改变转子叶片吸力面前缘分离涡损失大小。此外,导叶两端间隙分配变化可以改变嘴环叶片吸力面激波强度,并通过诱发交变载荷变化方式影响转子叶片可靠性。     

Reflection of a moving shock wave over an oblique shock wave

The reflection of a moving shock wave over a wedge immersed in a still gas and the reflection of a wedge induced steady shock wave over symmetrical and asymmetrical reflecting surfaces have received intensive considerations since more than 70 years ago. Here we consider a different shock reflection problem—reflection of a moving shock wave over an initially steady oblique shock wave induced by a wedge immersed in supersonic flow. For the flow condition we considered, five moving triple points, with each connecting an incident shock wave, a reflected shock wave and a Mach stem, are identified. By using the reference frame co-moving with each triple point, the type of each shock wave of this triple point is clarified. The present study is significant in that it treats a new shock reflection problem leading to a new shock reflection configuration and showing potential applications in supersonic flow with unsteady shock interaction.     

Influence of shock wave impinging region on supersonic film cooling

Shock waves can significantly affect the film cooling for supersonic flow and shock waves may have different influence when impinging in different regions. The present study numerically compared the results of shock wave impinging in three different regions and analyzed the effect of impinging region. The shock wave generators were located at x/s = 5, 25, 45 with 4°, 7° and 10° shock wave incidence. The mainstream Mach number was 3.2 and the coolant Mach number was 1.2 or 1.5. The numerical results illustrated that the shock wave impinged in the further upstream region led to a larger high-pressure region and a larger vortex in the boundary layer. Moreover, placing the shock wave generator upstream resulted in the lower mass fraction of coolant in the downstream region. The velocity in the upstream part of the cooling layer was lower than the midstream and downstream part, which resulted in the less ability to resist the shock wave impingement. Therefore, the upstream impingement deteriorated the cooling performance to a greater extent. The study also manifested that the stronger shock wave had a larger effect on supersonic film cooling. Increasing the coolant inlet Mach number can increase the blowing ratio and reduce the mixing, which was of benefit to improve cooling effect.     

Geoeffectiveness of interplanetary shocks controlled by impact angles: A review

The high variability of the Sun’s magnetic field is responsible for the generation of perturbations that propagate throughout the heliosphere. Such disturbances often drive interplanetary shocks in front of their leading regions. Strong shocks transfer momentum and energy into the solar wind ahead of them which in turn enhance the solar wind interaction with magnetic fields in its way. Shocks then eventually strike the Earth’s magnetosphere and trigger a myriad of geomagnetic effects observed not only by spacecraft in space, but also by magnetometers on the ground. Recently, it has been revealed that shocks can show different geoeffectiveness depending closely on the angle of impact. Generally, frontal shocks are more geoeffective than inclined shocks, even if the former are comparatively weaker than the latter. This review is focused on results obtained from modeling and experimental efforts in the last 15?years. Some theoretical and observational background are also provided.     

水下爆轰燃气泡形态与激波传播过程研究

针对脉冲爆轰发动机在水下工作过程中形成的燃气射流问题,搭建了水下爆轰燃气实验系统,研究了第一个爆轰循环中燃气泡发展变化过程.建立了基于气液两相双流体模型的脉冲爆轰发动机水下喷射模型,采用时-空守恒元和求解元方法,模拟了爆轰波与水相互作用形成的激波的传播及衰减过程.研究结果表明:燃气射流冲击水面时,燃气泡形态在膨胀阶段受...