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.     

基于值域的多约束GNSS单频单历元定姿新算法

多天线增强了全球卫星导航系统（GNSS）单频单历元姿态测量解算模型的强度,但随着天线数量增加,模糊度维数成倍增加,从模糊度域确定搜索空间的计算量将显著增长。基于此,提出了基于值域的多约束多天线GNSS单频单历元姿态测量新算法：该算法将姿态约束融入值域搜索模型,利用姿态约束条件推导搜索步长,通过姿态域三维搜索确定模糊度搜索空间,以基于最优条件姿态解非迭代近似估计的方法固定模糊度。实验结果表明,新算法中模糊度搜索效率较原方法提高约65.8%,固定模糊度效率较标准迭代算法提高约95.3%,且与标准迭代算法性能相当;所提算法能够实现GNSS单频单历元的模糊度固定和载体全姿态测量,具有较高的正确率。     

加载速率对层间断裂韧性的影响

虽然加载速率对层间断裂的影响已经被广泛的研究,但是现有的研究结果还未能给出加载速率对层间断裂韧性影响的明确趋势。研究人员发展了许多测量层合板复合材料以及胶接层断裂韧性的实验方法。本文的主要目的是对层间断裂韧性测量的实验方法进行综述,尤其是准静态和动态加载条件下层间起裂韧性的测量。首先介绍了准静态下Ⅰ型、Ⅱ型以及Ⅰ/Ⅱ复合型层间断裂韧性的测量方法,然后综述动态加载下层间断裂韧性的实验方法。前两部分着重介绍断裂实验中断裂参数(载荷、位移、起裂时间以及裂纹长度)的测量以及断裂韧性的计算。之后又综述了两种光学测量方法在层间断裂实验中的应用。最后将文献中加载速率对层间断裂韧性影响的实验研究结果进行了总结。     

Portfolios of promise: A review of R&D investment techniques and how they apply to technology development in space agencies

Despite a rich legacy of impressive technological accomplishments, the government acquisition of advanced space systems is increasingly synonymous with schedule slips and cost overruns. Program reviews have suggested that investing more in centralized and strategic research and development outside particular programs will reduce technical uncertainties and improve cost and schedule outcomes. This paper suggests roles for a centralized technology office by examining the methods available in the literature for managing portfolios of research projects.     

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.