电磁兼容实验室接地装置的设计与安装

合理地设计和安装接地装置对无线电实验室、电磁兼容实验室以及电磁屏蔽室等具有十分重要的意义。分析了影响接地线电阻和流散电阻的主要因素，提出了结合电磁兼容实验室的特殊要求接地线、接地体选取的方案以及通过土壤改良来降低土壤电阻率的具体措施，并简要阐述了接地装置安装施工的过程及接地电阻测量的方法。     

单向电永磁作动器结构优化与动态特性分析

针对电磁作动器的使用要求,设计出一种具有能耗低、吸力大及响应快等特点的新型单向电永磁作动器。结合有限元仿真软件,利用有限元法研究作动器的结构参数如铁芯齿形结构、平面结构、无永磁结构、铁芯的倾斜角度及衔铁位移（气隙厚度）等因素对作动器电磁吸力和响应速度的影响。结果表明,电磁吸力随着作动衔铁位移的增加而大幅度减小;倾角结构的铁芯设计能使作动器性能达到最佳,且铁芯的倾斜角度为50°时,电磁吸力有最大值3071N。     

线圈炮——电磁同轴发射器及其系统分析

线圈炮在宇航与国防中有重要应用前景。本文先简述其分析模型与方程。方程为非线性变系数常微分方程的初值问题，有时呈刚性。用Ｔｒｅａｎｏｒ方法求解，所得结果与国外已有装置的试验数据符合良好。并对一个小炮做了初步的原理设计。     

带传动实验机的电磁兼容性分析

本文主要对带传动实验机噪声的产生和传播途径进行了全面的分析，从而为设计、安装、调试和使用带传动实验机提供了技术支持。     

直9直升机机载数据传输电缆电磁耦合分析

通过对数据传输电缆的仿真分析计算,得到了传输信号频率、电缆回路之间的距离与电磁耦合之间的关系.对于直9系列直升机中数据传输电缆的物理模型计算结果表明,感应电压会在传输频率为75MHz时达到最大值,线间距离为1.5mm时具有最小值.分析结果为直9系列直升机/飞机机载数据电缆的布线优化和电磁兼容改进设计提供一定参考依据.     

TM波照射时喷气发动机进气道的极化散射矩阵

对ＴＭ波照射下喷气发动机进气道的极化散射矩阵进行了分析计算。通过将喷气发动机进气道等效成规则的圆波导腔结构，用多个波导模的叠加表示进气道内电磁场，并采用平面孔径辐射场的克希荷夫积分公式和电磁场互易定量，求得了进气道的极化散射矩阵，从而将复杂的腔体散射问题简化到只需求在规则波导模激励下喷气发动机终端的反射系数。所得结论对单、双站散射均适用。     

PML在三维柱坐标系下的应用及脉冲天线数值模拟

在三维柱坐标系下推导了麦克斯韦方程在完全匹配层 (PML )吸收边界条件中的时域有限差分 (FDTD)表达式 ,从而把 FDTD推广到三维复柱坐标系中并编程实现。为保证求解的稳定性 ,给出了更为严格的时间步长计算公式 ,并去除了对称轴上的奇点。提出了利用插值法对 PML最外层理想金属层进行设置的方法 ,并简化了通常处理理想金属表面电磁场的约束条件。最后给出在柱坐标系下脉冲天线的数值模拟。     

Stability and shape analysis of relative equilibrium for three-spacecraft electromagnetic formation

The invariant shapes for close formation flying with inter-craft electromagnetic force ensure several potential space applications. However, the 6-DOF relative equilibrium problem has not been systematically investigated. This paper mainly analyzes the invariant shapes of relative equilibrium for the three-spacecraft electromagnetic formation, and studies the families of invariant shape solutions with real and constant magnetic moments as well as their linear stability. The problem is examined based on the full nonlinear coupled dynamic models for collinear and general triangular configurations. The relative equilibrium conditions are analyzed to determine whether an invariant shape do exist, and the corresponding families of invariant shape solutions are identified for static and spinning configurations respectively. Finally, the linear stability of such invariant shapes is numerically discussed, which have shown that most invariant shapes are unstable and controllable.     

Electromagnetic Induction Effects and Dynamo Action in the Hermean System

Embedded in a large mass density and strong interplanetary magnetic field solar wind environment and equipped with a magnetic field of minor strength, planet Mercury exhibits a small magnetosphere vulnerable to severe solar wind buffeting. This causes large variations in the size of the magnetosphere and its associated currents. External fields are of far more importance than in the terrestrial case and of a size comparable to any internal, dynamo-generated field. Induction effects in the planetary interior, dominated by its huge core, are thought to play a much more prominent role in the Hermean magnetosphere compared to any of its companions. Furthermore, the external fields may cause planetary dynamo amplification much as discussed for the Galilean moons Io and Ganymede, but with the ambient field generated by the dynamo and its magnetic field-solar wind interaction.     

电磁超介质研究进展

电磁超介质是当前电磁学和物理研究领域中的前沿与热点，文章将左手材料、复合左／右手传输线、光子晶体统一在电磁超介质的体系下进行介绍，并论述了电磁超介质的发展现状。