激波冲击下Air/SF6斜界面不稳定性实验研究

激波在不同密度介质上的交互作用在可压缩湍流上具有重要的基础价值。激波在界面上的作用会引起Richtmyer-Meshkov不稳定性。激波不正规折射时,流场存在更多复杂的涡。研究马赫数为1.23、1.41的激波在初始倾角β=60°的Air/SF6界面上非正规折射的情况。入射激波的切向冲击和法向冲击的相互作用,在界面处产生涡,折射波在壁面发生马赫反射。利用阴影显示技术,给出了界面演化和混合的过程。     

基于CATIA二次开发的渐开线直齿轮参数化设计

实现了在CATIA二次开发平台上渐开线直齿圆柱齿轮的参数化三维造型.首先在屏幕对话框中输入齿轮的参数,然后程序对设计计算、数据处理、图形绘制等进行综合处理,最后在CATIA中生成齿轮的三维模型.     

复合材料层合曲板的非线性动力稳定性

建立了复合材料圆柱曲板受外压作用的大变形动力学控制方程。在边界夹支可移的条件下借用数值方法求得曲板中面随时间的响应历程。将动力响应与Ｂ－Ｒ准则相结合,给出了对称正交铺层复合材料曲板受均布突加外压作用的动态失稳“跳跃”特性图。讨论了铺层顺序和结构参数对曲板跳跃特性的影响。     

振荡环境下推进剂液滴亚临界蒸发响应特性

针对推进剂液滴在惰性气体中的蒸发过程建立了非定常物理模型,并应用全隐差分格式离散模型方程进行数值求解。研究了液滴蒸发过程对环境气体压力振荡的响应特性,可为液体火箭发动机不稳定燃烧分析提供理论基础。      

Falkner-Skan流空间演化的二次稳定性研究

依据Floquet理论建立三维亚谐扰动的控制方程，研究Falkner-Skan流的二次稳定性问题。采用高精度的谱方法进行数值模拟，结合边界层特性有效地配置边界条件，引入不同类型压力梯度，研究在压力梯度下的二维有限振幅的Tollmien-Schlichting（TS）波对三维亚谐扰动的产生、发展和演化的作用和影响。结果表明，顺压梯度的存在可以减缓二次不稳定的发生和演化，而逆压梯度却加速了二次不稳定性。     

核磁共振陀螺信号仿真及噪声分析

核磁共振陀螺具有体积小、精度高、功耗低等优势,有望成为下一代惯性导航系统的核心部件,目前正受到人们的广泛关注。比较全面的介绍了核磁共振陀螺的基本理论,在此基础上利用时间离散化方法推导并建立了能够充分考虑核磁共振陀螺系统动态特性的仿真模型。利用该模型研究分析了锁相环相位、磁场、温度以及探测光强在1×10-5均方根幅度下均匀白噪声对陀螺信号的影响,发现它们对角随机游走、零偏不稳定性影响依次减小,且都具有自身独特的频率响应特性。其中,锁相环相位噪声引起的角随机游走与零偏不稳定性分别为5.1985×102(°)/h1/2、3.4593×103(°)/h,而探测光强噪声引起的角随机游走与零偏不稳定性分别为3.1623×10-1(°)/h1/2、4.7603×10-1(°)/h。该研究对深入分析核磁共振陀螺动力学机理、寻找主要噪声来源、提高陀螺性能具有重要意义。     

某型航空活塞发动机排气门积铅机理

针对某型航空活塞发动机在含铅汽油条件下因排气门积铅而出现严重的气缸压缩性衰减问题,通过对排气门上沉积物的微观形貌及成分分析,结合该型发动机的结构设计和实际运行环境分析这种排气门沉积物的形成机理.研究表明:空中慢车时排气门运行温度过低是导致污染物在排气门上沉积的根本原因,而空中慢车时的螺旋桨风车因素和该型发动机燃油系统设计特性是导致排气门运行温度过低的主要原因。据此提出将螺旋桨风车转速降低200 r/min和小功率调贫控制排气温度在427 ℃以上等提高气门运行温度的方案,经实际运行测试有效。     

The Full Flowpath Analysis of a Hypersonic Vehicle

对一种类X43-A吸气式高超飞行器全流道开展了M7一级的三维数值仿真研究,深入探索了进气道处于起动状态和不起动状态时全流道的冷流流场结构和和气动力特性,且部分结果与实验数据进行了对比。研究结果表明:(1)前体横截面上存在显著的展向压强梯度,使得经过预压缩的气流偏离了进气道进口,但同时也减少了进入内通道的边界层气流,提高了进口流场的品质;(2)后体喷流股的膨胀过程受到了周围外流的显著干扰,因而沿流动方向其截面形状不断发生变化,如在喷口附近为近似矩形,而在后体末端附近则演化为近似三角形;(3)当进气道处于不起动状态时,其全流道流动结构发生了显著变化,进气道的外部压缩波系往复振荡,尾喷管出口的喷流股也在不停的膨胀和收缩,具有极强的非定常特征;(4)当进气道处于不起动状态时,全机的气动力特性呈周期性变化,升阻比的变化幅度较大,在最大、最小值分别可达起动状态的2倍和1/4倍。另外,升力、阻力系数的变化曲线之间存在一定的相位差;(5)与实验结果的对照表明,所采用的数值仿真方法具有较高的精度。     

Hydrodynamic instabilities and transverse waves in propagation mechanism of gaseous detonations

The present study examines the role of transverse waves and hydrodynamic instabilities mainly, Richtmyer–Meshkov instability (RMI) and Kelvin–Helmholtz instability (KHI) in detonation structure using two-dimensional high-resolution numerical simulations of Euler equations. To compare the numerical results with those of experiments, Navier–Stokes simulations are also performed by utilizing the effect of diffusion in highly irregular detonations. Results for both moderate and low activation energy mixtures reveal that upon collision of two triple points a pair of forward and backward facing jets is formed. As the jets spread, they undergo Richtmyer–Meshkov instability. The drastic growth of the forward jet found to have profound role in re-acceleration of the detonation wave at the end of a detonation cell cycle. For irregular detonations, the transverse waves found to have substantial role in propagation mechanism of such detonations. In regular detonations, the lead shock ignites all the gases passing through it, hence, the transverse waves and hydrodynamic instabilities do not play crucial role in propagation mechanism of such regular detonations. In comparison with previous numerical simulations present simulation using single-step kinetics shows a distinct keystone-shaped region at the end of the detonation cell.     

Heliopause stability revisited: dispersion analysis and numerical simulations

The heliopause, a surface separating the tenuous hot heliosheath flow and the dense, strongly magnetized interstellar flow, is subject to instabilities of the Rayleigh–Taylor and Kelvin–Helmholtz types. The dynamic evolution of this discontinuity is of considerable importance for understanding the neutral atom and cosmic-ray filtration at the interface. Here, we investigate the stability of the upwind heliopause in the presence of charge exchange collisions using both an analytic (dispersion relation) approach and a numerical model that includes the interstellar magnetic field. The linear analysis yields a cubic dispersion relation that admits imaginary solutions for the full range of wavenumbers, implying that the stagnation point on the heliopause is unconditionally Rayleigh–Taylor unstable to small perturbations propagating parallel to the discontinuity surface. We confirm this result by following the nonlinear development of the instability with a time-dependent simulation using a four fluid MHD-neutral numerical code. For the typical solar wind and LISM conditions, we obtain cyclical evolution of the upwind heliopause with a period of the order of 100 years. We also identify two areas of space physics where the instability may have important implications.