翼面隐身结构在飞航导弹模型上的数值仿真研究

隐身结构是指由蒙皮和多种内部材料组成的、能满足承载要求、并具有明显降低雷达散射截面的结构。目的是探讨在常规布局飞航导弹上采用隐身结构的效果。以某常规布局飞航导弹模型为背景，设计出两种翼面隐身结构方案，并将这两种翼面隐身结构方案分别应用于飞航导弹模型的弹翼。应用时域有限差分法（FD-TD法）建立了飞航导弹模型电磁散射数值模型。通过数值仿真手段，计算、比较和分析了含有翼面隐身结构的飞航导弹和普通全金属飞航导弹的RCS值。数值仿真结果显示，与普通飞航导弹相比，这两种翼面隐身结构在许多方位上均能有效降低飞航导弹的RCS值。     

利用分层测试实现无线电高度表故障诊断

针对早期无线电高度表可测性不强的问题 ,提出了分层测试的思想 ,以两种常见体制的无线电高度表为例 ,通过测试需求分析 .设计了切实可行的分层测试方案 ,从测试方法、内容、原理和结果分析等方面进行了描述。软件模拟运行表明 ,分层测试可明显提高测试深度和故障诊断率 ,有效解决高度表可测性差的问题 ,满足系统设计指标 ;相对于人工测试 ,可提高式作效率 ,缩短检测周期。     

基于DPSA的几种全极化RWR前端升级方案

现代高技术战争条件下，电子战任务和电磁环境中威胁信号形式变得更加多样复杂，要求电子战支援系统（ESM）天线传感器能够接收和检测各种不同极化的威胁信号，即具有全极化接收能力。本文首先简要的介绍了一种性能优良的天线一双极化曲折天线（DPSA），然后提出了利用单个双级化曲折天线，将现有机载雷达告警接收机升级为全极化接收机系统的四种解决方案，其中重点介绍了基于极化组合/分解思想的第四种方案。     

ABORT-like detector to combat active deceptive jamming in a network of LFM radars

This paper studies an electronic counter-counter measures (ECCM) scheme combating against deceptive electronic counter measure (ECM) techniques.An adaptive detector exploiting generalized likelihood ratio test (GRLT) criterion is applied to detect the presence of deceptive jamming in fractional Fourier transform (FrFT) domain.First,the generating mechanism of spurious frequencies is analyzed based on the Volterra serial.The proposed nonlinear distortion model based on power amplifier behavior is robust in distortion analysis when the memory effect is considered.Second,a modified adaptive beamformer orthogonal rejection test (ABORT) like detector in closed form is built.The proposed detector can discriminate the echo and deceptive jamming adaptively by exploiting primary data and secondary data.This ECCM scheme is capable of guaranteeing the performance without the restriction of orthogonality,which is essential for the ABORT detectors.The expansion to radar network is discussed as a special case at the final part of this paper.Numerical simulations demonstrate the effectiveness of the proposed method.     

螺旋桨目标的雷达回波信号相位解缠技术

建立了螺旋桨的雷达回波信号模型。对模型回波信号的相位混叠效应进行了理论分析,讨论了回波相位混叠效应出现的原因,通过模型改进获得了螺旋桨的雷达回波相位的理论表达式。提出插值与可调门限相结合的算法和自适应数值积分算法两种相位解缠方法,分别用于桨叶数为偶数和奇数时的相位解缠。仿真结果表明:两种算法有较高的精度。     

飞机机身近区电磁散射建模研究

采用物理光学法和一致性几何绕射理论，分析机身各 球面波照射下的近场电磁散射特性几何绕射并建立其雷达散射截面（ＲＣＳ）数学模型，同时对于复杂机身的前部，采用面元油、即采用双三次Ｂ样条技术对机外形进行拟合，然后再用一致性几何绕射理论进行计算。种方法具有一定的可信度。     

220GHz频率步进雷达测距的实验研究

频率步进雷达是一种典型的高分辨雷达,它可以通过瞬时窄带合成宽带实现距离向的高分辨的同时降低A／D和其他设备的负担。文章介绍了220GHz频率步进雷达的工作原理和测距的方法,并对不同距离处的角反射器进行探测。实验结果表明,太赫兹雷达对角反射器距离向的探测距离精度可以达到厘米量级;同时,还对太赫兹雷达的探测距离进行了验证,最远探测距离可达35m。     

Plasma and electromagnetic wave simulations of meteors

Every day billions of meteoroids impact and disintegrate in the Earth’s atmosphere. Current estimates for this global meteor flux vary from 2000 to 200,000 tons per year, and estimates for the average velocity range between 10 km/s and 70 km/s. The basic properties of this global meteor flux, such as the average mass, velocity, and chemical composition remain poorly constrained. We believe much of the mystery surrounding the basic parameters of the interplanetary meteor flux exists for the following reason, the unknown sampling characteristics of different radar meteor observation techniques, which are used to derive or constrain most models. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. We present our results on meteor plasmas simulations of head echoes using particle in cell (PIC) ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body. We also present the results of finite difference time domain electromagnetic simulations (FDTD), which can calculate the radar cross section of the simulated meteor plasmas. These simulations have shown that the radar cross section depends in a complex manner on a number of parameters. These include the angle between radar and meteor entry, a large dependence on radar frequency, which shows that for a given meteor plasma size and density, the reflectivity as a function of probing radar frequency varies, but typically peaks below 100 MHz.     

基于通用数字信号处理器的雷达坐标测量系统

介绍了由PC机主CPU与TMS320C32(以下简称C32)DSP构成的多目标雷达坐标测量系统，并将任务合理分配给PC机主CPU及C32负担，从而使PC机主CPU和C32在低价位下提供最佳性能。     

Comparison of mesopause region meteor radar winds,medium frequency radar winds and low frequency drifts over Germany

During 2004 and 2005 measurements of mesospheric/lower thermospheric (80–100 km) winds have been carried out in Germany using three different ground-based systems, namely a meteor radar (36.2 MHz) at the Collm Observatory (51.3°N, 13°E), a MF radar (3.18 MHz) at Juliusruh (54.6°N, 13.4°E) and the LF D1 measurements using a transmitter (177 kHz) at Zehlendorf near Berlin and receivers at Collm with the reflection point at 52.1°N, 13.2°E. This provides the possibility of comparing the results of different radar systems in nearly the same measuring volume. Meteor radar winds are generally stronger than the winds observed by MF and especially by LF radars. This difference is small near 80 km but increases with height. The difference between meteor radar and medium frequency radar winds is larger during winter than during summer, which might indicate an indirect influence of gravity waves on spaced antenna measurements.