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.     

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。     

三线阵相机在轨温度场分析

文章依据"资源三号"卫星三线阵相机在轨工作环境特点,简要分析了三线阵相机热控设计的难点,给出了相应的解决措施,分析并总结了相机的在轨温度场,以相机在轨温度数据验证相机热控设计的正确性。结果表明,相机在轨温度稳定,所有温度均能满足指标要求,证明相机热控设计合理正确。     

叶片全三维反问题优化设计方法

基于数值求解Navier-Stokes方程,对叶轮机械叶片全三维反问题优化设计方法进行研究.反问题给定叶片表面的静压分布反求叶型,假设叶表网格点有虚拟移动速度,迭代过程中根据叶表的实际静压和目标静压之差来修改叶型.对单排叶栅进行了反问题设计,并给出了初步的优化算例,结果能很好地满足目标静压分布,验证了该方法的有效性,计算的时间和精度也适合进行工程应用.      

非对称喷管超声速流场的PIV实验与数值模拟

选取了跟随性能以及散射性能都上佳的二氧化钛粒子,利用了粒子图像测速仪(particle image velocimetry,PIV)对不同落压比下的非对称喷管(single expansion ramp nozzle,SERN)流场进行了测量,成功获取了相应流动结构,以及沿程上壁面压力分布和速度场等.在测得的图像中,可以清晰地观察到由于过膨胀产生的激波与膨胀波系,并进一步获得出口速度分布.运用计算流体动力学数值模拟方法,对实验状态下的非对称喷管进行了模拟.对比结果发现:PIV实验测得流场结构能很好地与其吻合,这互相验证了CFD计算和PIV实验的正确性及可靠性.      

An alternative Shell inversion technique - Analysis and validation based on COSMIC and ionosonde data

Multi-channel Global Positioning System (GPS) carrier phase signals, received by the six low Earth orbiting (LEO) satellites from the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) program, were used to undertake active limb sounding of the Earth’s atmosphere and ionosphere via radio occultation. In the ionospheric radio occultation (IRO) data processing, the standard Shell inversion technique (SIT), transformed from the traditional Abel inversion technique (AIT), is widely used, and can retrieve good electron density profiles. In this paper, an alternative SIT method is proposed. The comparison between different inversion techniques will be discussed, taking advantage of the availability of COSMIC datasets. Moreover, the occultation results obtained from the SIT and alternative SIT at 500 km and 800 km, are compared with ionosonde measurements. The electron densities from the alternative SIT show excellent consistency to those from the SIT, with strong correlations over 0.996 and 0.999 at altitudes of 500 km and 800 km, respectively, and the peak electron densities (N_mF₂) from the alternative SIT are equivalent to the SIT, with 0.839 vs. 0.844, and 0.907 vs. 0.909 correlation coefficients when comparing to those by the ionosondes. These results show that: (1) the N_mF₂ and h_mF₂ retrieved from the SIT and alternative SIT are highly consistent, and in a good agreement with those measured by ionosondes, (2) no matter which inversion technique is used, the occultation results at the higher orbits (∼800 km) are better than those at the lower orbits (∼500 km).     

基于纹理的活动轮廓三维图像分割研究

对具高噪声和低对比度三维图像的识别和分割算法进行了研究。基于活动轮廓模型,用Gabor变换提取图像的纹理特征,根据统计学信息假设,通过偏微分方程水平集和窄带方法求解,获得较基本活动轮廓的算法分割更光滑精确的物体轮廓。实验结果表明:改进模型算法的效率和准确度达到预期效果。     

3D雷达对3D雷达的引导提示性能分析

分析了不同位置关系3D雷达对3D雷达的成功引导概率及引导误差,讨论了成功引导概率随参数特征变化的性质,仿真分析目标到提示雷达不同斜距时目标在被提示雷达中的角度分布及引导误差变化。研究对雷达组网中3D雷达对3D雷达引导提示系统设计有一定的参考价值。