中等高超声速弹体头,尾形状对气动性能影响的实验研究

六种常规弹体在两种细长比下头部和尾部形状时CN,Xcp的影响进行实验研究，实验名义Mach数为4．0，4．5，5．0和6．0，a＝0°～6°（或0°～8°）。获得了一些对高超声速飞行器研制有实用价值的结果。     

关于刚体转动的角速度和角加速度的讨论

在理论力学教学中，平面运动刚体的转动与基点无关的证明过于简单，本利用矢量代数的知识，证明平面运动刚体的角度与角加速度与基点的选择无关。     

细长体分离起始点的实验研究

本文实验研究了细长体模型在中等迎角下的初始分离问题。观察了不同头部形状的细长体在不同迎角下的分离流态。考察并分析了分离起始点的性质。观察到开式分离的存在,实验结果分析认为开式分离可以起始于正常点。此外,在钝头和尖头模型上都出现了螺旋点形式的头部涡。它们或是闭式分离的起始点,或是奇点型开式分离的起始点。     

超声速燃烧室凹腔火焰稳定器的数值模拟

为分析凹腔火焰稳定器在超声速燃烧室中的流动特性,运用数值模拟方法研究了凹腔对H2超声速燃烧的作用规律。通过对比分析不同凹腔长深比L/Du,后缘倾角θ,后缘深度Dd和H2喷射位置Ljet对燃烧室性能的影响,发现凹腔的火焰稳定机制主要在于富含自由基的高温回流区;L/Du=7~9,θ=30°,Du/Dd=1.0和Ljet=24mm的燃烧室强化混合燃烧的性能较好,可以获得较高的燃烧效率和总压恢复。     

The multifuid solar wind termination shock and its influence on the threedimensional plasma structure upstream and downstream

The solar wind termination shock is described as a multi-fluid phenomenon taking into account the magnetohydrodynamic self-interaction of a multispecies plasma consisting of solar wind ions, pick-up ions and shock-generated anomalous cosmic ray particles. The spatial diffusion of these high energy particles relative to the resulting, pressure-modified solar wind flow structure is described by a coupled system of differential equations describing mass-, momentum-, and energy-flow continuities for all plasma components. The energy loss due to escape of energetic particles (MeV) from the precursor into the inner heliosphere is taken into account. We determine the integrated properties of the anomalous cosmic ray gas and the low-energy solar wind. Also the variation of the compression ratio of the shock structure is quantitatively determined and is related to the pick-up ion energization efficiency and to the mean energy of the downstream anomalous cosmic ray particles. The variation of the resulting shock structure and of the solar wind sheath plasma extent beyond the shock is discussed with respect to its consequences for the LISM neutral gas filtration and the threedimensional shape of the heliosphere.     

环形燃烧室性能计算

在任意曲线坐标系下对包括扩压器和火焰筒在内的环形燃烧室三维两相反应流进行了数值模拟。燃烧室性能采用多维经验分析法估算所用的数学模型有 κ-ε,紊流模型 ,EBU -Arrhenius紊流燃烧室模型 ,六通量热辐射模型以及颗粒群轨道模型。在非交错网格体系下 ,气相采用 SIMPLE算法和液相采用 PSIC算法求解 ,通过两种工况和三种扩压器进口速度分布计算表明 ,所得的流场各气流参数分布和燃烧室性能较合理 ,本文所建立的程序可为燃烧室优化设计和研制提供有用数据。     

侧向喷流的一种直接实验模拟

研究了侧向喷流的一种直接实验模拟技术,旨在探讨喷流力直接作用在天平上时,侧向喷流对气动载荷的影响及其增益情况。本文的直接模拟是通过一种通气式应变天平实现的。研究中分析了有关模拟原则,妥善处理了诸如高压气体密封、天平变形引发的漂移、干扰等相关技术问题,并在一尖拱柱构型上实现了多种条件下的直接模拟,给出了来流条件和喷口参数条件对法向力、俯仰力矩增益因子的影响。最后,就实验结果进行了适当讨论和评述。     

考虑高载和阻尼介质时刚塑性圆板的塑性动力分析

本文研究了阻尼介质对刚塑性圆板在高载(冲击荷载)作用下塑性动力响应的影响,得到了解析解并对此解进行了讨论。当阻尼介质参数趋于零时,本文结果与无阻尼解一致。文中还画出了荷载与阻尼介质对圆板运动时间和板中心点残余挠度的影响曲线。     

行星际空间MHD模拟激波跃变关系分析

分析了模拟得到的可以传播到1AU以远的日地空间磁流体力学激波与Rankine-Hugnoniot跃变关系的符合程度．通过对模拟激波的结构及其在传播过程中的演化进行的分析，提出了模拟激波的定位方法；基于所提出的定位方法，利用向长青提出的确定MHD激波局地参数的方法计算了模拟得到的激波与Rankine-Hugnoniot跃变关系的偏差．结果表明在激波传播到100Rs以后，激波对中前向快激波与Rankine-Hugnoniot关系的符合达到很高的程度，相对误差在10^-2数量级以内；并且在激波传播到150 Rs以后，相对误差在10^-3数量级以内．这个结果说明文中所使用的有限差分数值格式能较好地模拟激波．     

Transonic buffet control research with two types of shock control bump based on RAE2822 airfoil

Current research shows that the traditional shock control bump (SCB) can weaken the intensity of shock and better the transonic buffet performance.The author finds that when SCB is placed downstream of the shock,it can decrease the adverse pressure gradient.This may prevent the shock foot separation bubble to merge with the trailing edge separation and finally improve the buffet performance.Based on RAE2822 airfoil,two types of SCB are designed according to the two different mechanisms.By using Reynolds-averaged Navier-Stokes (RANS) and unsteady Reynolds-averaged Navier-Stokes (URANS) methods to analyze the properties of RAE2822 airfoil with and without SCB,the results show that the downstream SCB can better the buffet performance under a wide range of freestream Mach number and the steady aerodynamics characteristic is similar to that of RAE2822 airfoil.The traditional SCB can only weaken the intensity of the shock under the design condition.Under the off-design conditions,the SCB does not do much to or even worsen the buffet performance.Indeed,the use of backward bump can flatten the leeward side of the airfoil,and this is similar to the mechanism that supercritical airfoil can weaken the recompression of shock wave.