某型无线电高度表灵敏度超差故障分析及排除

针对某型无线电高度表在进行总体测试中经常出现灵敏度超差这一故障现象，对测试原理和工作原理进行分析，并提出利用防泄磁装置对电耦合器进行防护的解决方案。     

2μm波段单频拉曼光纤放大器中受激布里渊散射研究

2μm波段高功率单频拉曼光纤放大器(SF-RFA)的性能通常会受到受激布里渊散射(SBS)效应的影响.本文考虑SBS效应下拉曼光纤放大器的速率方程,建立了SBS限制下的SF-RFA理论模型,计算了SF-RFA的能量分布和功率输出.讨论了泵浦功率、光纤长度等因素对光纤放大器中SBS效应和输出功率的影响,总结了如何在提高放大器输出功率的同时有效抑制SBS效应的方法.本文数值模拟结果为实验研究高功率SF-RFA中抑制SBS效应提供一定的指导.     

四元数最小均方误差算法及其在波束形成中的应用

 作为多维信号处理的一个重要工具,四元数代数已在各个领域有所应用。对四元数最小均方误差(QMMSE)算法进行了研究,首先推导了四元数实数形式的最小均方误差(QRMMSE)算法,进一步推导了四元数复数形式的最小均方误差(QCMMSE)算法,并且分析了两种算法的区别和计算量。最后将QMMSE算法应用到机载简化矢量传感器阵列的波束形成中,与复数长矢量最小均方误差(LVMMSE)算法相比较,QCMMSE算法的性能有所提高,计算量有所减少。计算机仿真结果验证了所提算法的有效性。     

星载二次电源的电磁兼容预设计

针对星载二次电源电磁兼容试验中辐射发射的超标问题,提出了电磁兼容预设计方法.分析二次电源电磁干扰产生的机理,利用SPICE仿真器建立传导干扰的电路等效模型,优化电路设计得到传导干扰源;应用修正的单线模型近似计算辐射干扰,根据计算结果,利用遗传算法优化等效偶极子的数目和分布位置建立场等效模型;基于场路结合的方法,以传导干...     

多输入多输出电磁矢量阵列雷达的DOD和DOA联合估计

研究一种基于电磁矢量传感器阵列的多输入多输出(MIMO)雷达目标波离角(DOD)和波达角(DOA)的联合估计算法.提出了一种新型MIMO雷达系统,发射阵列采用常规阵元,而接收阵列采用电磁矢量传感器,在此基础上,算法首先利用矢量传感器的内在结构特点结合子空间旋转不变性质获得目标DOA预估计,随后采用最佳加权子空间拟合算法...     

地线设计在PCB电磁兼容性中的作用

简介了电磁兼容性(EMC)的基本概念,并结合某项目实际应用,说明地线设计的一点改变即可在PCB电磁兼容方面起到重要作用.     

基于优化加权高分辨距离像的雷达目标识别(英文)

对雷达目标高分辨距离像进行特征加权可以解决高分辨距离像各距离单元因目标姿态变化而导致的稳定性不一致问题。针对已有加权系数求解方法存在的不足,提出一种加权系数优化方法。该方法通过定义目标函数来度量不同雷达目标之间加权高分辨距离像的可分性,并采用梯度下降算法优化加权系数值,从而达到增强高分辨距离像稳定距离单元作用,减小不稳定距离单元影响的目的。基于5种飞机目标模型高分辨距离像的仿真实验表明,该方法可以有效优化加权系数,并提高雷达目标识别率。     

机载箔条弹雷达回波的建模与仿真

飞机目标通常抛撒箔条弹来干扰雷达的工作。针对这一作战场景,首先研究分析了飞机与箔条的运动特性和雷达回波特性,导出了对于地基防御雷达而言,箔条弹在时域上可视为点目标、在多谱勒域上可不考虑其多谱勒展宽效应的结论。在此基础之上,建立了箔条干扰的数学和仿真模型,模拟并分析了飞机加箔条的运动状态和雷达回波特性。研究成果有助于揭示箔条干扰的雷达特性,评估箔条的干扰效果。     

X-Rays From Mars

X-rays from Mars were first detected in July 2001 with the satellite Chandra. The main source of this radiation was fluorescent scattering of solar X-rays in its upper atmosphere. In addition, the presence of an extended X-ray halo was indicated, probably resulting from charge exchange interactions between highly charged heavy ions in the solar wind and neutrals in the Martian exosphere. The statistical significance of the X-ray halo, however, was very low. In November 2003, Mars was observed again in X-rays, this time with the satellite XMM-Newton. This observation, characterized by a considerably higher sensitivity, confirmed the presence of the X-ray halo and proved that charge exchange is indeed the origin of the emission. This was the first definite detection of charge exchange induced X-ray emission from the exosphere of another planet. Previously, this kind of emission had been detected from comets (which are largely exospheres) and from the terrestrial exosphere. Because charge exchange interactions between atmospheric constituents and solar wind ions are considered as an important nonthermal escape mechanism, probably responsible for a significant loss of the Martian atmosphere, X-ray observations may lead to a better understanding of the present state of the Martian atmosphere and its evolution. X-ray images of the Martian exosphere in specific emission lines exhibited a highly anisotropic morphology, varying with individual ions and ionization states. With its capability to trace the X-ray emission out to at least 8 Mars radii, XMM-Newton can explore exospheric regions far beyond those that have been observationally explored to date. Thus, X-ray observations provide a novel method for studying processes in the Martian exosphere on a global scale.     

Planar laser scattering visualization of streamwise vortex pairs in a Mach 6 flow

A series of cross-sectional flow fields of Counterrotating Vortex Pairs(CVPs) generated by a large-scale ramp vortex generator is observed using an ice-cluster-based Planar Laser Scattering(PLS) method in a shock tunnel with a nominal flow Mach number of 6. Combined with a numerical simulation, two streamwise CVPs with opposite rotating directions are identified in the wake flow of the vortex generator with an absence of a boundary layer, namely, a Primary CVP(PCVP) and a Secondary CVP(SCVP). Th...