Unsteady experimental and numerical investigation of aerodynamic performance in ultra-high-lift LPT

Detailed experimental and numerical investigations were performed for an ultra-high-lift front-loaded low-pressure turbine cascade (Zw = 1.58) with periodic wakes. The interaction mechanisms between the incoming wakes and endwall secondary flow were carefully examined. Wakes were produced by moving upstream rods, and flow field downstream of the cascade was measured using a seven-hole probe. Experimental results revealed that incoming wakes influenced not only the boundary layer development of the blade suction surface but also the complex endwall secondary vortex structures. On the suction surface: Incoming wakes clearly suppressed the suction side separation bubble at a low Reynolds number of 25000. Nevertheless, the effects of different wake passing frequencies were not significantly different at Re = 100000, and the profile losses under wake passing were even greater than in the absence of wakes. At the endwalls: Incoming wakes more strongly suppressed secondary flow at Re = 100000 than at Re = 25000, because the low-momentum fluid inside the incoming wakes clearly increased the endwall cross-passage pressure gradient at Re = 25000. The experimental results indicated that periodic wakes decreased the passage vortex and counter vortex core strength by 25% and 30%, respectively, at Re = 100000. Instantaneous results also demonstrated that endwall secondary vortices decreased significantly near the position of wakes passing.     

稀薄效应对可倾瓦动压气体轴承性能的影响

以微型三可倾瓦动压气体轴承为研究对象,采用连续模型、一阶滑移模型和WU新滑移模型速度边界条件,建立考虑稀薄效应的滑移修正雷诺方程。结合牛顿迭代法和有限差分法求解修正雷诺方程,计算考虑稀薄效应的三可倾瓦动压气体轴承各瓦块压力分布和承载力。计算结果表明:三可倾瓦动压气体轴承偏心率越大,转速越大,压缩系数越大,轴承承载力越大;考虑稀薄效应后,计算出的可倾瓦动压气体轴承承载力明显下降,且随着克努森数的增大,WU新滑移模型计算得到的承载力明显低于一阶滑移模型。     

跨声速叶栅通道中叶片压力面簸箕孔型气膜冷却特性

在跨声速叶栅通道内,试验研究了叶片压力面气膜冷却特性,详细地对比分析了在不同主流进口雷诺数(Re=17×105,37×105,57×105)、出口马赫数(Ma=081,091,101)及多个气膜吹风比(M=05～30)条件下的压力面簸箕孔型气膜冷却效率。试验结果表明:主流出口马赫数变化对气膜孔下游冷却效率的分布与具体数值均无影响;而主流进口雷诺数的影响较大。增大主流进口雷诺数使得气膜分离再贴附对应的吹风比相应增大,Re=17×105时在吹风比M=10时出现气膜分离与再贴附现象,而Re=37×105和Re=57×105对应的临界吹风比则分别为20和25;主流进口雷诺数越大,小吹风比下近孔区域的冷却效率越高,而在孔下游区域则相反;大吹风比下,则主流进口雷诺数越大冷却效率越小。     

大视场红外星敏感器折反式光学系统设计

星敏感器是以恒星为探测对象的高精度空间姿态测量装置,广泛应用于卫星、航天飞机、导弹等必备的高精度姿态敏感部件。为了实现在特定环境要求下的精确应用,本文设计了可应用于近红外波长的红外光学系统。首先,根据既定的参数进行了初始结构的选型,并对马克苏托夫望远镜的形式进行了改进。然后,对设计结果进行了探测性能分析。随后对设计好的系统进行了公差分析及优化,使它能满足加工装配需求。最后,为光学系统设计了遮光罩,进行了杂散光分析。设计与分析结果表明：该探测光学系统折反射镜全表面采用球面,系统总长171.2mm,全视场14μm包围能量分布均在86%以上,0.8视场内最大畸变小于4μm。该系统视场大、结构紧凑、装调难度低、探测灵敏度高、探测范围广、温度适应性强,可在0.8～1.9μm近红外波段的宽光谱范围内进行高精度目标检测的准确检测。     

S形进气道流路造型方法及其对性能影响的研究

根据S形进气道的几何边界条件,提出了一种基于多项式的中心线及面积分布率曲线的流路造型方法。选择不同的拐点位置,采用该方法构造了9条具有代表性的中心线及面积分布率方程。组合不同的中心线和面积分布率曲线建立了相应的S形进气道的几何造型,并采用三维N-S方程进行求解,得到了总压恢复系数和DC60等性能指标。分析计算结果表明,中心线对S形进气道总压恢复和出口动压起着主要影响,随着中心线方程拐点位置后移,S形进气道总压恢复系数和出口动压呈明显增加趋势;中心线和面积分布率组合共同影响着DC60指标,当中心线拐点过于靠近进气道进口而面积分布率曲线拐点靠近进气道出口时,进气道下游的涡将会发展到出口,从而大幅度影响DC60指标。     

二元超声速进气道流管压缩量特性与应用初步研究

为研究流管压缩程度与超声速进气道临界总压恢复系数的规律,以双楔外压式进气道为例,对不同来流马赫数、多种方案进行实例研究。研究马赫数范围为2.0至4.0,各种压缩方案涉及宽泛的总转折角范围和多种楔角组合方式。研究结果表明,就通常设计中常用的压缩方案范围而言,临界总压恢复系数与流管收缩比呈明显的正相关变化规律,并在一定的范围内两者呈近似线性关系,基于流管收缩比可实现对临界总压恢复系数大小的近似判断。      

调压阀快速开关定位控制算法研究

介绍了针对某车载气动试验设备中配置的特种高压调压阀而开发的一种控制算法,目的是将调压阀用于快速开关定位控制与压力调节双重任务。配置有快速阀和调压阀的系统,对调节过渡时间有严格的要求。调压阀用于根据实际系统工艺的要求,改变调压阀后的压力,以跟踪系统气源压力的变化。快速阀用于快速接通系统工作介质。由于受车载空间限制,通过本方案的改造,可以使系统不需使用快速阀,减小系统空间的占用,适合车载系统等对空间要求苛刻的场所。笔者提出的调压阀快速开关控制算法,经过实际验证,证明方法可行,效果良好,满足实际的需要。     

壁面带微结构管道内Cassie状态稳定性的实验研究

保持液体在微结构表面处于Cassie状态,是流动减阻的关键。首先利用MicroPTV分别测量了带微结构侧壁处于Cassie和Wenzel状态下的流场速度,表明Cassie状态下近壁速度提高至光滑表面的1.6倍,而Wenzel状态下近壁速度将减小。通过精细控制微管道的驱动压强,观察了液体在近壁由Cassie向Wenzel状态的转变,并测出C/W转变的临界压强值Δpcr约10.9kPa,与Laplace理论预测值10.15kPa基本相符。考虑到Cassie状态失稳也会发生在液体进样过程中,实验还观察了微结构角点对液体进样的＂锚定＂作用,并初步分析了液体进样中自由液面在微结构表面保持Cassie状态的条件。     

Propagation of cylindrical and spherical dust–ion acoustic solitary waves in a relativistic dusty plasma

The properties of cylindrical and spherical dust–ion acoustic solitary waves (DIASW) in an unmagnetized dusty plasma comprising of relativistic ions, Boltzmann electrons, and stationary dusty particles are investigated. Under a suitable coordinate transformation, the cylindrical KdV equation can be solved analytically. The change of the DIASW structure due to the effect of geometry, relativistic streaming factor, ion density and electron temperature is studied by numerical calculation of the cylindrical/spherical Kdv equation. It is noted that with ion pressure the effect of relativistic streaming factor to solitary waves structure is different. Without ion pressure, as the relativistic streaming factor decreases, the amplitude of the solitary wave decreases. However, when the ion pressure is taken into account, the amplitude decreases as the relativistic streaming factor increases and is highly sensitive to relativistic streaming factor. Our results may have relevance in the understanding of astrophysical plasmas.     

VASIMR中螺旋波等离子体源设计

螺旋波等离子体具有密度高,可控性强且无电极等优点,被应用于可变比冲磁等离子体火箭(VASIMR,Variable Specific Impulse Magnetoplasma Rocket)中.设计了一个螺旋波等离子体源,并给出了其中2个关键部分——磁场线圈和螺旋波天线的设计.对螺旋波等离子体源进行了初步实验,结果表明,电子密度随射频输入功率的增加几乎呈线性上升,估计电子密度的量级在通入工质后完全可达10¹¹ cm^-3.