基于CFD高精度算法的雷电电磁场研究

雷电空间电磁场一直是电磁领域研究的热门，成熟的算法例如有限时域差分法（FDTD），传输线矩阵法（TLM）以及频域的矩量法（MoM）在计算雷电问题方面都有广泛的应用。由于计算流体力学（CFD）中的Euler方程与电磁学中的Maxwell方程有着相同的守恒形式，而且采用间断伽辽金方法（DG）已经在流场问题上得到广泛的尝试，因此引入了基于计算流体力学的DG方法来离散时域Maxwell方程，并采用网格分区并行技术加速计算，使用基于DG的圆球雷达散射截面积（RCS）算例进行测试，数值结果一致表明DG算法在求解电磁场问题上的可行性，之后通过计算一段近场雷电通道的电场分布并与解析解、某算法仿真解对比，数据基本吻合，说明该方法适合于雷电电磁场的计算。     

抗辐照通用扩展SiP芯片设计

研究微小卫星综合电子系统的SiP技术实现方法。首先介绍微小卫星综合电子系统结构的组成和采用SiP技术的必要性，然后对综合电子系统进行功能模块划分，并对其通用扩展模块进行详细的SiP设计，包括抗辐照器件选型、原型验证、SiP原理图、基板管壳一体化设计、建模仿真、制造加工、实装测试验证等，通过SiP技术实现了一种星载综合电子系统中通用扩展SiP芯片产品，经过实际验证测试，在保证模块功能和性能的前提下，整体模块重量从230 g减轻到48 g，体积由180 mm?130 mm?17 mm减小到46 mm?46 mm?8 mm，很好地满足了星载功能模块小型化、轻量化设计需求。     

战术导弹折叠翼快速展开性能的测试技术

介绍某些战术导弹折叠翼快速展开特性测试技术。详细地介绍了测量方法、项目、数据处理和主要结果。试验是在北京空气动力研究所一座低速风洞中进行的。试验结果表明，获得的数据具有很高精度和可靠性，重复性也是令人满意的。     

原子时自动测量及数据采集系统

介绍了普通的时间实验室的时频测量,实现自动测量和数据收集的基本系统方案,并以上海天文台原子时实验室为例介绍了实际可行的自动测量和数据收集系统,这个系统高性能、低价格,可应用于国内几乎所有的时间实验室。     

表贴式永磁电机的两种充磁方式

研究了表贴式永磁电机的两种充磁方式。首先利用已有文献电机参数验证了有限元模型的正确性,对比分析了两种充磁方式下电机磁密和磁钢磁势的分布特点,研究表明内转子结构平行充磁方式具有提供更大的气隙磁通潜力,而外转子结构则相反。接着研究了两种充磁方式,不同气隙下气隙总磁通随极对数和磁钢厚度的变化规律。同时明确了两种充磁方式各自使用场合,给出了最佳磁钢厚度的取值范围。本文工作有助于正确选择表贴式永磁电机的充磁方式和磁钢厚度,以发挥磁钢潜力,改善电机性能。     

Solar and Heliospheric Modulation of Galactic Cosmic Rays

The significance of external influences on the environment of Earth and its atmosphere has become evident during recent years. Especially, on time scales of several hundred years, the cosmogenic isotope concentration during the Wolf-, Spoerer-, Maunder- and Dalton-Minimum indicates an increased cosmic ray flux. Because these grand minima of solar activity coincide with cold periods, a correlation of the Earth climate with the cosmic ray intensities is plausible. Any quantitative study of the effects of energetic particles on the atmosphere and environment of the Earth must address their transport to Earth and their interactions with the Earth’s atmosphere including their filtering by the terrestrial magnetosphere. The first problem is one of the fundamental problems in modern cosmic ray astrophysics, and corresponding studies began in the 1960s based on Parker’s cosmic ray modulation theory taking into account diffusion, convection, adiabatic deceleration, and (later) the drift of energetic particles in the global heliospheric magnetic field. It is well established that all of these processes determining the modulation of cosmic rays are depending on parameters that are varying with the solar magnetic cycle. Therefore, the galactic cosmic ray intensities close to Earth is the result of a complex modulation of the interstellar galactic spectrum within the heliosphere. The modern view of this cosmic ray modulation is summarized in our contribution.     

Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton

We present an analysis of seven clusters observed by XMM-Newton as part of our survey of 17 most X-ray luminous clusters of galaxies at z  0.2 selected for a comprehensive and unbiased study of the mass distribution in massive clusters. Using the public software FTOOLS and XMMSAS we have set up an automated pipeline to reduce the EPIC MOS and pn spectro-imaging data, optimized for extended sources analysis. We also developped a code to perform intensive spectral and imaging analysis particularly focussing on proper background estimate and removal. XMM-Newton deep spectro-imaging of these clusters allowed us to fit a standard β-model to their gas emission profiles as well as a standard MEKAL emission model to their extracted spectra, and test their inferred characteristics against already calibrated relations.     

全天球实时恒星模拟器技术

阐述了研制全天球实时恒星模拟器的意义以及国内外发展趋势,介绍第二代恒星模拟器的系统组成、特点、技术指标以及解决的技术问题。     

基于DRFM的引信干扰技术研究

根据脉冲测距引信的工作原理和DRFM的基本功能,设计了DRFM结构,DRFM通过对脉冲延时,达到对脉冲测距引信进行干扰使其早炸的目的,并提出了延时参数的确定原则。