浅析光学测量方法在修理企业零件制造方面的应用

介绍了应用光学测量方法还原无图零件、铸造件、磨损件以及测绘零件三维模型的方法，运用数控加工、增材制造等加工方法，实现了无图样零件的制造和检测。     

Modified micro-mechanics based multiscale model for progressive failure prediction of 2D twill woven composites

To consider fiber random distribution at the microscale for the multiscale model based on the micro-mechanics failure (MMF) theory, clustering method is used for the extraction of amplification factors. As the clustering method is a kind of unsupervised machine learning method, the elements with similar mechanical behavior under external loading can be included in a cluster automatically at the microscale. With this modification, the fiber random distribution model can be used for multiscale damage analysis in the framework of MMF theory. To validate the modified multiscale analysis method, progressive damage analysis of a kind of 2D twill woven composites is conducted based on different microscale models. The stress values for microscale models with fiber hexagonal and random distribution patterns are compared first. Much higher stress concentration is generated in the fiber random distribution model due to the smaller inter-fiber distance especially under longitudinal shear loading. The obtained cluster distribution results exhibit the characters of the stress distribution in the two microscale models. Thereafter, tensile and compressive responses of the 2D twill woven composite are predicted with the modified multiscale analysis method and accuracy of the method is verified through comparison with published experimental results. From the simulation results, it can be found that the matrix damage initiation from the model based on the fiber random distribution model is premature compared with that from the model based on the fiber hexagonal distribution model. Besides, under tensile loading, the damage all initiates from the fill tows and propagates to the wrap tows. However, under compressive loading, the matrix damage initiates from the wrap tows in the model based on the fiber random distribution model.     

考虑气穴影响的2D压力伺服阀稳定性

为研究双自由度（2D）压力伺服阀工作时的气穴现象对阀芯稳定性的影响，利用AMESim中的基本库和HCD库建立2D压力伺服阀各组件仿真模型。理论分析得出气穴现象会降低阀体中含气油液的有效体积弹性模量，得出考虑气穴影响的阀芯稳定性条件。仿真结果表明气穴现象会导致主阀芯到达稳定位置后出现振荡现象，影响主阀芯的穿越频率从21 Hz降低至6 Hz，限制主阀芯的频宽，适当增加主阀芯阻尼比能提高主阀芯工作稳定性。提出一种新型阻尼活塞结构，建立模型分析得出其能在不影响伺服阀频响、阀芯位移和抗污染能力情况下提高主阀芯阻尼比以提高阀芯工作稳定性，并且设计实验进行验证。实验结果表明，应用阻尼活塞将2D压力伺服阀压力输出波动从9%降低至2%，能够提高飞行器制动时刹车阀工作稳定性。     

Temporal evolution of the EIA along 95°E as obtained from GNSS TEC measurements and SAMI3 model

The total electron content (TEC) derived from GNSS measurements at a trans-hemispheric meridional chain of ground stations around 95°E longitude are used to study the quiet time inter-hemispheric structure and dynamics of the equatorial ionization anomaly (EIA) during the period March 2015 to February 2016. The stations are Dibrugarh (27.5°N, 95°E, 43° dip), Kohima (25.6°N, 94.1°E, 39° dip), Aizawl (23.7°N, 92.8°E, 36° dip), Port Blair (11.63°N, 92.71°E, 9° dip) and Cocos Islands (12.2°S, 96.8°E, 43° dip). The observation shows that the northern crest of the EIA lies in the south of 23°N (Aizawl) in all seasons but recedes further south towards the equator during December solstice. The largest poleward expansion of the northern (southern) EIA is observed in the March equinox (December solstice). The equinoctial and hemispherical asymmetry of TEC is noted. The winter anomaly is observed in the northern hemisphere but not in the southern hemisphere. The highest midday TEC over any station is observed in the March equinox. The TEC in southern summer (December solstice) is significantly higher than that in the northern summer (June solstice). The observed northern EIA contracts equatorward in the postsunset period of solstice but the southern EIA persists late into the midnight in the December solstice. The asymmetry may be attributed to the different geographic location of the magnetically conjugate stations. The SAMI3 simulations broadly capture the EIA structure and the inter-hemispheric asymmetry during solstices. The difference between observations and the SAMI3 is higher in March equinox and December solstice. The higher E?×?B vertical drift in the 90–100°E sector and the large geographic-geomagnetic offset in observing stations may have contributed to the observed differences.     

基于三维激光成像系统的相机标定方法

三维激光成像系统中点云数据与影像数据的融合可以对被扫描物体赋予真彩色.为了获得点云数据与影像数据良好的融合效果,就需要精确的确定载体坐标系与相机坐标系之间的关系.本文针对三维激光成像系统点云模型真彩色处理方法进行研究,提出了一种基于三维激光成像系统的相机标定方法.通过对相机坐标系的标定,建立点云数据与影像数据之间的数学模型.实验结果显示,采用所提出的方法,能够使得三维立体点云数据与影像数据精确融合.最终得到被扫描目标的真彩色3D模型.     

嫦娥三号动力落月段轨迹确定策略

针对CE-3（嫦娥三号）月球探测器动力下降弧段,特别是悬停避障段频繁机动的特点,提出了采用B样条函数逼近方法进行落月轨迹确定.仿真分析表明：在动力下降运动较平滑弧段,B样条逼近法计算结果略优于多项式拟合法;而在频繁机动弧段,B样条逼近法有明显优势.计算结果表明,加入VLBI（Very Long Baseline Interferometry,甚长基线干涉测量）数据后能有效提高落月轨迹确定精度,在没有系统误差的情况下联合定位后位置精度优于50 m.此外,还分析了三向测量系统差对定位的影响,可对CE 3任务提供参考.最后对CE 3实测数据进行处理,动力落月段末点位置和着陆器定位计算值相差不到200 m.     

一种光学遥感成像系统优化设计新方法研究

针对空间光学高分辨率遥感器,既要实现轻小型化,又要获得高品质遥感图像的要求,文章提出一种空间光学遥感成像系统优化设计新方法;综合考虑成像链路各环节因素,采用全面的指标设计和合理的优化设计流程来改进空间光学遥感成像系统的总体指标和成像品质,并显著降低遥感器的研制难度.通过比较全链路优化设计方法和传统设计方法的仿真结果及其...     

微小卫星雷达隐身性能的在轨逆合成孔径雷达成像验证

成像雷达是空间目标监视系统中的重要组成部分.为深入评估某微小卫星的隐身性能,对卫星的逆合成孔径雷达(ISAR)成像效果进行预测,从雷达成像角度评估卫星的隐身效果.首先简述用于空间目标成像的ISAR成像的基本原理.然后构造卫星的散射点模型,散射系数采用微波暗室的实际测量值.依据仿真雷达系统参数和卫星实际在轨运行参数,计算卫星ISAR成像所需成像时间.对卫星3种飞行姿态,即卫星顶部指向地球表面的隐身姿态、卫星顶部与飞行方向一致和卫星底部指向地球表面两种非隐身姿态,以及不同信噪比情况,进行ISAR仿真,详细分析每种情况下的运动补偿效果和最终ISAR成像效果,说明了卫星隐身设计的有效性.     

ISAR非平稳目标成像时间和转速联合估计方法

针对逆合成孔径雷达(ISAR)非平稳目标成像,提出基于两特显点相位联合估计成像时间和转速的方法,并得到了转速与相位斜率差(PSD)的解析表达式.首先,基于两个特显点距离单元估计目标转动相位,根据不同时间段转动相位线性度(PLD)选择成像时间.其次,在适合成像的时间段,将成像时间等分成两段,分别提取两段时间内转动相位的斜...