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.     

白天激光漫反射测距中微弱信号检测的单开门多触发方法

白天激光漫反射测距因存在强背景噪声,导致微弱回波信号的检测十分困难,严重限制了激光漫反射测距的广泛应用。因此,提出了采用单开门多触发方法解决白天激光漫反射测距的微弱信号检测难题。首先,介绍了一种GM-APD (Geiger-ModeAvalanchePhotoDiode,盖革模式雪崩光电二极管)多触发概率分布函数的快速求解方法。接着,取激光漫反射测距系统典型参数,理论分析了多触发情况下的回波信号检测概率,分析结果表明单开门多触发方法可提高激光漫反射测距在白天情况下的回波信号检测概率。同时,通过对触发次数限制的优选,可以增加有效检测比,减少白天观测条件下回波信号的提取代价。最终,通过系统仿真验证了理论分析结果的正确性。因此,单开门多触发方法是解决白天激光漫反射测距微弱信号检测的可行途径之一。     

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.     

用于基带雷达引信的平面等角螺旋天线的特性与设计

通常希望一个天线的波瓣图和阻抗能在一个较工的频率范围内保持不变。我们将这一类称为非频变天线。平面等角螺旋天线是一这一类天线的典型例子。本文主要叙述了平面等角螺旋天线的宽频带特性和工作原理，并简要介绍了它的设计方法。     

天线雷达散射截面的分析与实验

本文利用天线散射的基本原理，以波导激励振子抛物面天线为例，计算并分析了天线的结构项散射雷达截面ＲＣＳｓ和模式项散射雷达截面ＲＣＳｅ，给出了此天线雷达截面的预估值。实验结果表明，理论预估值与实测值吻合较好，并且证明天线的模项ＲＣＳｅ大于结构项ＲＣＳｓ，天线总的雷达截面主要受天线模式散射的影响，减小模式项ＲＣＳｅ将有效地降低天线的雷达截面。本文结果为探索以克服天线模式散射为主的天线ＲＣＳ减缩技术提供了理论依据