车身三坐标检测数据图形分析软件开发

根据三坐标测量机检测汽车车身后输出的数据特点,提出了一种计算机图形分析方法,并介绍了软件的编制.实施后,大大减少了车身精度分析时间,提高了分析准确性,并有效地提高了白车身质量.     

HyTRV流场特征与边界层稳定性特征分析

高超声速转捩研究飞行器（HyTRV）是为研究三维复杂外形的边界层转捩问题而设计的一款具备真实飞行器典型特征的升力体标模。为支撑更加全面系统的理论分析、数值模拟、风洞试验和飞行试验研究,采用高精度数值模拟方法、线性稳定性理论（LST）和e^N方法对HyTRV标模的典型流动特征和边界层失稳特征进行了分析。研究表明,HyTRV展现出多个相对独立的横流区域和多个流向涡结构;HyTRV的边界层存在横流失稳模态、第二模态、附着线失稳模态等常见模态。横流失稳模态出现在周向高低压区之间的横流区域,能够主导转捩发生;横流区域同时也存在第二模态,其N值普遍比横流失稳模态小;附着线失稳模态呈现出第二模态特性,且频率非常高。还研究了攻角和单位雷诺数的影响。结果表明,随着攻角增加,标模下表面中心线的流向涡结构逐渐消失,横流雷诺数逐渐减小;上表面流向涡结构逐渐从腰部移向顶端,并出现新的流向涡结构。增加攻角,所有失稳模态的N值总体上逐渐减小;增加单位雷诺数,N值显著增加。基于研究结果,针对流向涡失稳、横流失稳、第二模态和附着线失稳等给出了研究建议。     

高超声速升力体飞行器等离子体鞘数值模拟

为探究高超声速再入过程中通信“黑障”的影响因素,基于一种化学反应平衡气体组分模型,采用有限体积法求解三维全N-S方程,数值方法采用AUSMPW+格式和LU-SGS隐式求解方法,模拟典型球锥体的高超声速流场,得到的电子数密度分布同RAM-C II飞行试验数据吻合良好。并针对一种升力体外形飞行器进行计算,选取高度范围35~55〖KG*9〗km、马赫数12~25、攻角10°~30°共14个飞行状态,得到了不同状态下的飞行器周围的电子数密度分布情况,对比分析发现电子数密度值与飞行高度、马赫数以及攻角的大小关系密切。     

基于伪谱法的小天体最优下降轨迹优化方法

针对小天体着陆探测下降阶段的多约束轨迹优化问题,基于Gauss伪谱法进行了燃耗最优下降轨迹优化设计,得出了燃耗最优下降轨迹。建立了小天体下降轨迹优化问题的最优控制问题模型,采用Gauss伪谱法进行离散化,转化为非线性规划问题进行了求解。数学仿真结果显示:优化结果符合各项约束条件,以零速度到达了目标着陆点,且符合燃耗最优的优化目标。利用Gauss伪谱法进行小天体最优下降轨迹优化,计算速度快,求解精度高。     

Preliminary experiment on spontaneous ignition performances of cavity-based strut flameholder

The thermal-structural response and low cycle fatigue life of a three-dimensional (3D) channel wall nozzle with regenerative cooling were numerically investigated by coupling the finite volume fluid-thermal method, nonlinear finite element thermal-structural analysis and local strain methods. The nozzle had a high area ratio (nozzle exit area divided by throat area) under cyclic working loads. Parametric studies were carried out to evaluate the effects of channel structural parameters such as channel width, channel height, liner thickness and rib width. Results showed that the integrated effects of three-dimensional channel structure and load distribution caused serious strain, which mainly occurred at the intersectant regions of liner wall on the gas side and the symmetric planes of channel and rib. The cooling effect and channel structural strength were significantly improved as the channel width and height decreased, leading to substantial extension of the nozzle service life. On the other hand, the successive decrease in liner thickness and rib width apparently increased the strain amplitude and residual strain of channel wall nozzle during cyclic work, significantly shortening the service life. The present work is of value for design of the channel wall nozzle to prolong its cyclic service life.      

“嫦娥二号”卫星拓展试验轨道计算中心天体的选取

飞行器的星历积分不可避免涉及中心天体的选取问题。“嫦娥二号”卫星在拓展试验期间处于弱引力区,文章针对拓展试验期间的轨道状态,从受摄运动二体问题角度分析得出适宜选取太阳作为中心天体。进而结合真实力模型情况,使用行星星历表计算行星产生的摄动力,从理论上推导得出在忽略小天体摄动的前提下,由于摄动天体同时对中心天体和飞行器产生摄动作用,以地球为中心天体产生的摄动力类似于潮汐力,而以太阳为中心天体则不然,因而更适宜选取地球作为中心天体计算轨道运动问题     

高风速下介质阻挡放电等离子体气动激励抑制翼-身组合体失速分离的试验研究

在较高风速下研究介质阻挡放电等离子体气动激励对翼一身组合体绕流流动的控制效果。结果表明：在来流风速100m／s的情况下,介质阻挡放电等离子体气动激励能较好地抑制流动分离,失速迎角推迟约30％,升阻比最大提高80％。研究结果为等离子体流动控制技术的应用奠定重要基础。     

基于BP神经网络的航空发动机装配参数对整机振动影响的研究

运用BP神经网络方法建立数学模型,研究装配参数对整机振动的影响,进而实现对整机振动参数的预测。试验研究表明,所建模型具有较高的预测精度。     

改进的粒子滤波算法在软着陆小天体中的应用

针对小天体软着陆过程中估计目标天体质心视线的导航方法失效问题,给出了一种基于特征点信息的自主光学导航方法。为了进一步提高对轨道参数的估计精度,考虑到系统中存在的非高斯噪声,以及基本粒子滤波算法带来的粒子退化和采样枯竭问题,给出了一种改进的粒子滤波算法。最后,通过仿真计算,验证了所给出的自主光学导航方法以及改进的粒子滤波算法的可行性和有效性。     

Dynamics in the Phobos environment

The dynamical environment on and about the Martian moon Phobos is explored. This planetary moon provides a unique dynamical environment in the solar system, being subject to extreme tidal forces and having a characteristically non-spherical shape. Further, it is not in a fully circular orbit, meaning that it has librations that arise from its eccentricity, contributing to a periodic forcing environment. Thus, to plan and implement missions in the vicinity of and on Phobos will require these considerations be taken into account. In this paper the latest published models of the Phobos shape and dynamics are used to characterize its dynamical environment in close proximity orbit about the body, for motion across its surface and for controlled hovering motion in its vicinity. It is found that surface motion is subject to a number of “speed limits” that can cause a moving vehicle to leave the surface and to possibly escape the moon and enter orbit about Mars. In terms of orbital stability, the existence of libration orbit families are characterized down to the surface using an exact potential, and the known stable QSO orbits are shown to be associated with families of stable quasi-periodic orbits.