H2O2-PE固液火箭发动机低频不稳定燃烧研究

介绍了85％H2O2-PE固液火箭发动机的低频不稳定燃烧特征;应用发动机质量守恒方程对发动机低频耦合振荡燃烧现象进行了一维模拟,分析了氧化剂喷射压降对低频不稳定燃烧的影响。利用扰动分析确立了固液火箭发动机的稳定工作限。提出了抑制低频耦合振荡燃烧的方法。     

Two-stream instability generation in the lunar ionosphere

The Two-stream Instability (TSI) generation is studied analytically in the lunar ionosphere. The TSI is a tiny perturbation in the electron plasma density, due to which an electric field grows with time and this growth is facilitated by the electron plasma in the background. In lunar ionosphere, the TSI comes into existence when the solar wind interacts unhindered with the tenuous lunar electron plasma in the surface bound exosphere. In this study, the conditions which allow the TSI to form and the subsequent instability growth with time i.e. the growth factor, is estimated. Initially, the threshold condition for the TSI to take place is determined. Thereafter, the solar wind and lunar plasma parameter contribution to trigger TSI is investigated along with the effect of these parameters in the evolution of TSI. The plasma TSI evolution with the passage of time is also depicted in phase space diagram with Particle-In-Cell simulations.     

Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.     

加筋壁板大开口结构稳定性分析及试验验证

为了研究加筋壁板大开口结构的压缩承载极限问题,规划了两组具有不同设计参数的试验件进行了静力试验,并同时采用了线性特征值法以及非线性的弧长法对其压缩极限进行了对比分析。在采用弧长法分析时,引入了模态扰动技术,而且考虑了材料的弹塑性性质。计算结果与试验的对比表明:针对复杂结构稳定性问题,屈曲特征值法具有较大局限性,而结合模态扰动的弧长法对这种复杂的加筋壁板类结构压缩极限的分析精度较好。通过分析给出了加筋壁板大开口结构设计的一些建议。     

螺旋桨桨叶1P气动载荷研究

介绍了一种１Ｐ载荷实验研究方法－桨叶应变测试法,首先通过桨叶剖面速度三角形及气动力分析给出了１Ｐ载荷与测量应变的关系,然后通过地面试验和飞行试验进行了验证。试验结果表明,螺旋桨１Ｐ载荷主要由于非对称气流流过桨盘面改变了桨叶剖面速度三角形而引起,迎角,侧滑角的增加,会产生较大的１Ｐ载荷;机动飞行,如快速拉杆,荷兰滚等也会产生较大的１Ｐ载荷。     

K8V变稳飞机飞行试验验证系统

介绍了Ｋ８Ｖ变稳飞机飞行试验验证系统的组成及功能,分别阐述了该系统的飞控软件综合验证子系统、机上地面试验数据采集与处理子系统和飞行试验数据处理分析子系统等三部分的组成、工作原理、以及在飞行试验各个阶段的不同特点和作用。通过Ｋ８Ｖ变稳飞机飞行试验的应用,表明该系统能够满足变稳飞机的软件维护、系统验收试飞及后续的应用研究,具有实时,快速,准确,自动化等优点,可为Ｋ８Ｖ变稳飞机应用研究提供重要的支持手段     

三维不可压边界层抛物化稳定性方程的椭圆特性研究

针对三维平行不可压边界层流动的抛物化稳定性方程,研究其剩余的椭圆特性,提出了消除该特性的具体方法,并对抛物化稳定性方程解与全椭圆问题解的一致性进行了证明。     

改善反作用轮低速性能的补偿观测器方法

基于Ｄａｈｌ摩擦模型,给出了用于卫星姿态三轴稳定控制的反作用轮低速动力学方程,就反作用轮转速过零对卫星姿态产生的扰动现象进行了分析,提出了一种利用非线性观测器估计摩擦力矩,并予以补偿的补偿观测器方法。仿真结果表明,该方法改善了反作用轮低速性能,提高了卫星姿态控制的指向精度和稳定度。     

基于抓持稳定度的多指灵巧手抓持控制

提出了一种控制多指灵巧手稳定抓持物体的新方法。首先给出了接触稳定度和抓持稳定度的定义及其相应的计算方法,然后探讨了基于抓持稳定度的多指灵巧手抓持控制方法。最后以北京航空航天大学的BH-2新型三指灵巧手为背景,对所提出的方法进行了仿真验证,仿真结果证明所提方法是有效可行的。     

大攻角风洞自由飞动导数实验研究

实验是在0.2×0.2m~2超音速风洞中进行的,其来流Mach数为2.0。模型为带翼导弹模型。实验时用气体发射装置将模型向实验段上游发射;并以另一气流横吹模型使其呈大攻角状态飞行。最大攻角可达100°。采用高速鼓轮相机记录模型飞行姿态随时间的变化。用改进的数值积分法进行数据处理,求得俯仰阻尼导数随攻角的变化。