超宽带射频仿真系统中的低RCS三轴转台设计

提出了在超宽带射频仿真系统中三轴转台的低RCS设计方法.该方法采用转台机械结构设计、低RCS外形优化分析与测试测量相结合的方式.首先基于低RCS要求及三轴转台的结构特性,对其进行外形优化.通过计算三轴转台的表面感应电流分布,分析三轴转台的强散射区域,并选取相应吸波材料及涂敷方法对三轴转台进行处理.实际测量表明,涂敷吸波材料后三轴转台散射回波幅度显著减小,分布均匀,达到了预设的效果.     

无线电引信抗海杂波干扰方法

无线电引信抗海杂波的能力决定了舰空导弹无线电引信低空和超低空工作性能,针对海杂波对无线电引信的影响,分析了海面回波的平均功率、海面散射系数、海杂波的多普勒频谱等海杂波特性,提出了无线电引信抗海杂波干扰方法。     

Pulsar radio emission

25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms P0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission. New are details of the preferred magnetic structure, wind generation, and amplification of the emitted (pseudo) curvature radiation, the inferred brightness of which exceeds that of all other terrestrial and astrophysical sources by many orders of magnitude.     

X-ray and radio observations of the galaxy cluster 3C 129

The galaxy cluster 3C 129 contains two radio galaxies, the prototypical head tail radio galaxy 3C 129 and the weaker radio galaxy 3C 129.1. The tail of the first radio galaxy extends over more than 15′ across the sky. In this paper, we report on Chandra spectroscopy observations of the galaxy cluster, complemented by new and archival radio data taken with the Very Large Array (VLA) at 0.33, 1.4, 5, and 8 GHz and by HI-observations performed with the dominion radio astrophysical observatory (DRAO). We describe the Chandra results on the properties of the Intra-Cluster Medium (ICM) and discuss extended X-ray emission detected from the host galaxy of the radio galaxy 3C 129.1 and from the inner jet of the radio galaxy 3C 129. Finally, we report on the results of an ICM/radio plasma pressure balance study along the tail of the radio galaxy 3C 129.     

光学加工射频离子源的去除函数与稳定性研究

在研究了射频离子源的结构、工作原理和性能的基础上,进行了光学镜面抛光离子束的去除效率与稳定性测试。实验结果表明射频离子源去除函数的形状为回转高斯形,利用Φ15mm的栅网,在靶距为30mm、离子能量900eV时,去除函数的峰值去除率为194nm/min,体积去除率为19.2×10-3mm3/min,半峰全宽值为9.2mm;并且去除函数的峰值去除率与体积去除率的变化均在3%以内,半峰全宽值的变化在1.7%以内。因此,射频离子源具有光学镜面抛光加工所需的去除效率,而且射频离子源具有好的稳定性,具备光学加工的潜能。     

Non-Gaussian clutter characterization applied to OTHR using a mixture of two Rayleigh probability density functions

A practical technique for characterizing non-Gaussian radar clutter is specified and demonstrated using Over The Horizon Radar (OTHR) data, as an example. The technique employs maximum likelihood to fit the probability density of the clutter amplitude returns to a mixture of two Rayleigh probability densities instead of the single Rayleigh density typically used for Gaussian clutter. This model for non-Gaussian clutter is fully specified for any set of clutter amplitudes by a log likelihood, two Rayleigh parameters, and a mixing coefficient. A 3D plot of these values yields an easily-visualized clutter characterization, as is illustrated using OTHR data. This technique is a demonstration of clutter characterization using OTHR data, but the method can be applied to characterize other types of clutter data.     

民用无线电发射信号对电磁环境的影响

对世界范围内的典型民用无线电业务进行了归纳分析,在空域、时域、频域和能量域等详细参数计算的基础上,分析了民用发射信号对电磁环境中电子设备接收机的影响,并提出了多种建议方法以最大限度地减小民用发射信号对电子设备系统设计的影响。     

无线电引信海面及目标多普勒回波仿真分析

频谱识别技术利用海面及目标回波的多普勒频差来滤除海杂波信号。为准确分析弹目交会时引信回波的多普勒频谱,采用了三维弹目交会模型对弹目不共面时引信回波进行模拟,利用等多普勒线划分海面区域进而计算海面回波多普勒频率,利用目标不同散射点合成的方法推导了目标回波多普勒频率的表达式,并在弹目飞行速率、弹目交会角及目标脱靶量等因素不同时对引信回波多普勒频率进行仿真,通过仿真分析得出了以上因素对引信回波多普勒频率的影响,并验证了频谱识别技术在不同交会条件下的有效性。     

非确定-确定混合分群算法及其实现

在最小群变化(LeastClusterChanged,LCC)分群算法的基础上提出一种非确定-确定混合(Uncer tainy CertainyMixed,UC CM)分群算法。该算法利用非确定性分群的竞争特性,提高了网络的初始收敛速度,并保持了LCC算法的稳定性,同时利用优先级参数,提高了组网的灵活性。设计了UC CM算法的有限状态机模型,并基于模型对算法进行了模拟仿真,验证了算法的有效性。     

电离层对单频卫星导航系统伪距差分定位的影响

用计算机仿真方法 ,给出了单频卫星导航系统伪距差分后 ,定位误差受电离层影响的一些结果。伪距差分定位能够校正电离层时延误差 ,但校正精度随用户与基准站到同一颗卫星倾斜因子的不同而不同。为此 ,提出了一种改进的伪距差分方法。仿真结果表明 ,改进后有明显效果