整级环境下涡轮叶片型面加工几何偏差影响的不确定性分析

加工等过程中产生的几何偏差会导致涡轮叶片气动性能及工作状态发生显著变化,对该影响的准确评估与合理分析具有重要意义.本文提出了一种考虑三维型面几何偏差对气动性能影响的不确定性计算分析方法,包括随机叶型几何建模、不确定性量化计算和敏感性分析等,并结合某一单级高压涡轮进行分析.基于随机过程理论和主成分分析法,参考现有叶片加工...     

单幅图像的三维重构视觉系统特征点提取算法的研究与实现

实现基于单幅二维图像不标定欧氏重构三维场景的关键技术之一是有效提取彩色伪随机编码图像特征角点。为给图像特征点匹配提供更多的样本信息,采用定位于彩色图像Harris算子探测特征角点,并动态给出角点响应的自适应阈值条件。特征点提取实验及三维欧氏重构结果证实了该方法的适用性和有效性。     

Validation on MERSI/FY-3A precipitable water vapor product

The precipitable water vapor is one of the most active gases in the atmosphere which strongly affects the climate. China's second-generation polar orbit meteorological satellite FY-3A equipped with a Medium Resolution Spectral Imager (MERSI) is able to detect atmospheric water vapor. In this paper, water vapor data from AERONET, radiosonde and MODIS were used to validate the accuracy of the MERSI water vapor product in the different seasons and climatic regions of East Asia. The results show that the values of MERSI water vapor product are relatively lower than that of the other instruments and its accuracy is generally lower. The mean bias (MB) was ?0.8 to ?12.7?mm, the root mean square error (RMSE) was 2.2–17.0?mm, and the mean absolute percentage error (MAPE) varied from 31.8% to 44.1%. On the spatial variation, the accuracy of MERSI water vapor product in a descending order was from North China, West China, Japan -Korea, East China, to South China, while the seasonal variation of accuracy was the best for winter, followed by spring, then in autumn and the lowest in summer. It was found that the errors of MERSI water vapor product was mainly due to the low accuracy of radiation calibration of the MERSI absorption channel, along with the inaccurate look-up table of apparent reflectance and water vapor within the water vapor retrieved algorithm. In addition, the surface reflectance, the mixed pixels of image cloud, the humidity and temperature of atmospheric vertical profile and the haze were also found to have affected the accuracy of MERSI water vapor product.     

某新型改性双基推进剂的热安全性

采用热重分析仪( TG)、差示扫描量热仪( DSC)以及加速量热仪( ARC)研究了一种以高氯酸铵( AP )为氧化剂的新型改性双基推进剂GATo-3的热安全性,并将实验结果与双基发射药SF-3进行了比较。通过TG/DSC实验得到了GA-To-3的热分解过程,并初步分析了AP等组分对其热稳定性的影响。 DSC的测试结果显示,GATo-3的2个分解峰温分别为180.5℃和187.7℃,低于SF-3的分解峰温;ARC的测试结果显示,GATo-3在理想绝热条件下的起始分解温度为129.1℃,绝热温升为1177.8℃,最大温升速率为58053.5℃/min,最大压力上升速率为52.5×105 Pa/min,单位质量生成气体的最大压力为112.4×105 Pa/g,用速率常数法计算活化能E=116.8 kJ/mol和指前因子A=5.1×1011 s-1,最大反应速率达到时间为24 h时,所对应起始温度TD24=74.0℃。研究结果表明,与双基发射药SF-3相比,GATo-3的热安全性较差,爆炸性较强。     

中点箝位型光伏并网逆变器调制策略及效率对比

传统三电平中点箝位(Three-level neutral point clamped,3L-NPC)半桥逆变器在高压大功率条件下,由于开关器件损耗不均衡而使其容量受限,因此衍生了多种NPC型三电平半桥拓扑。为了优化选取NPC型拓扑及调制策略,对4种3L-NPC型拓扑(二极管NPC、有源式NPC、层叠式NPC及有源层叠式NPC)的调制策略及开关器件损耗分布进行了对比分析,并研制了一台5kW的NPC型统一实验平台,进行了效率测试。理论分析与实验结果表明:(1)根据零电平续流路径的配置不同,NPC型拓扑主要有4种调制策略;(2)选取合理的NPC型拓扑及调制策略,不仅可以均衡器件损耗,而且系统效率基本不变,为逆变器的扩容奠定了基础。     

Analytic and numerical treatment of motion of dust grain particle around triangular equilibrium points with post-AGB binary star and disc

This paper investigates the motion around the triangular equilibrium points, of a passively gravitating dust particle in the gravitational field of a low-mass post-AGB binary system, surrounded by circumbinary disc. The two bodies of the binary are modeled as a triaxial star and a radiating-oblate star. Due to small deviation of disc stars on circular orbits, we have assumed that the Coriolis and centrifugal forces of the stars are slightly perturbed. The triangular equilibrium points of the particle are found. These points are defined by, triaxiality of the primary star, oblateness and radiation of the secondary one and the gravitational potential from the disc mass. Further, when the disc mass increases, the particle moves nearer to the stars and farther away from the disc. In general, these equilibrium points are linearly stable when μ < μ_C; where μ is the mass ratio and μ_C is the critical mass function, defined by the parameters of the system. The effects of each of these parameters on the size of the stability region are stated, and the periodic motion around the stable points is examined. It is seen that the orbits are ellipses, and the orientation, eccentricities, lengths of the semi-major and semi-minor axes are influenced by the parameters of the problem. In particular, for our numerical linear stability analysis, we have taken an extremely depleted pulsating star, IRAS 11472-0800 as the post-AGB triaxial star, with a weakly-radiating young white dwarf star; G29-38 as the secondary. For this system, the stability result of the triangular points comes out different. Here, μ_C < μ throughout the entire range of the mass ratio and the critical mass function. Hence, the triangular equilibrium points are unstable. The stability of the orbits is tested using the Poincaré surfaces of section (Pss). The region of stability is controlled by the introduced parameters and the Jacobi constant.     

复合材料在长焦距空间光学遥感器上的应用

对碳纤维增强聚合材料(CFRP)和碳化硅颗粒增强铝基(SiCp/Al)复合材料在空间光学遥感器的应用进行了介绍,并以某长焦距空间光学遥感器的主支撑结构为例,对应用不同材料时遥感器的质量、固有频率、热位移等进行了研究。研究结果表明:应用复合材料能够使主支撑结构质量降为278kg,从而降低发射成本;结构具有较大的刚度,固有频率为156.09Hz,满足设计指标;可以更加有效控制结构热变形引起的光学元件刚体位移,提高成像品质。文章对复合材料更好地应用于长焦距空间光学遥感器,具有一定的参考价值。     

基于星载毫米波顺轨-交轨InISAR的空间运动目标三维成像技术研究

研究了低信噪比情况下的星载毫米波顺轨/交轨In\|ISAR空间目标三维成像问题。由于传统的RD成像算法在目标尺寸较大和分辨率要求较高时不能取得较好的成像效果,故将波数域成像算法引入运动目标成像处理以获得高分辨率的二维图像,继而将顺轨/交轨三天线ISAR图像分别进行干涉处理,获得了目标上各散射点的三维位置。作为二维成像、图像配准等重要环节的基础参数,对低信噪比下的目标检测和三维运动参数估计进行了研究,分析了速度估计精度要求。最后,仿真结果表明了顺轨/交轨In-ISAR系统的有效性。