渐变体微波散射截面的计算

对具有二维周期性结构特点的大尺寸金属渐变体,首先采用矩量法计算渐变体单元的散射场,然后利用天线阵列技术求解整个渐变体的雷达散射截面RCS (Radar Cross Section),既保证一定的计算精度,又解决计算量大以及单元间耦合的难题.推导了相关的数学公式,在线极化平面波入射情况下,分别给出了单个和多个金属渐变角锥电磁散射截面的计算例子,计算结果与商用软件HFSS (High Frequency Structure Simulator)计算得到的结果相吻合,计算用时大大少于HFSS的计算时间,表明介绍的方法在工程运用上是可行的.      

一种基于DCT的SAR图像自聚焦算法

研究了一种基于离散余弦变换(DCT, Discrete Cosine Transform)的SAR(Synthetic Aperture Radar)图像自聚焦算法.该方法从复图像域出发,通过在距离压缩相位历史域引入相位误差模型,改变图像的聚焦程度直至一维像的DCT序列在高序数区域的权值达到最大,从而完成误差校正.同相位梯度自聚焦算法相比,该方法无需在图像域分离出强点目标,因此特别适用于无任何明显特征的图像.由于DCT存在快速算法,使得该自聚焦算法计算量较少,更易实现.实测数据及仿真数据的成像结果证明了此方法的可行性.      

基于DDS任意波形发生器的研究

基于DDS原理设计了一种任意波形发生器,并通过软件编程实现对其频率字和参考频率的改变,以提高波形发生器输出信号频率的准确性。     

智能化雷达对抗情报处理技术研究

随着雷达技术的迅猛发展,雷达信号的密度、复杂程度都大幅度提高,这就增加了雷达信号的不确定性因素。本文讨论了粗糙集理论、模糊集理论、证据理论和可能性理论等人工智能技术在雷达对抗情报处理中的应用。对雷达辐射源的型号和工作模式识别、雷达网信息以及所属平台信息的推理技术进行了探索研究,给出了研究建议。     

软件雷达技术研究综述

从较为成熟的软件无线电技术出发,介绍了软件雷达的基本概念、通用结构、通用信号处理平台和适用于软件雷达的数据结构,总结了软件雷达的优越性能和发展趋势。     

Orbit insertion error analysis for a space-based gravitational wave observatory

Constellation is required to be highly stable over several years for a space-based gravitational wave observatory. However, the stability of the constellation can be affected by orbit insertion errors. The effects of orbit insertion errors on the constellation are mainly studied in this paper. Firstly, Monte-Carlo, Unscented Transformation Covariance Analysis Method (UTCAM) and Spherical Simplex Unscented Transformation Covariance Analysis Method (SSUTCAM) are used for simulation. The results indicate that UTCAM and SSUTCAM are highly efficient in calculating, with a relative error of less than 6%. Therefore, it is concluded that because of their accuracy and high efficiency, UTCAM and SSUTCAM can be adequately used in orbit insertion error analysis for a space-based gravitational wave observatory. Secondly, SSUTCAM is used to study the effects of position and velocity errors on the constellation. For the case in this paper, when the position error does not exceed 300 km, and the velocity error does not exceed 4 cm/s, the constellation remains stable.     

不同半径圆柱诱导CH4/空气预混燃烧的计算研究

本文研究不同半径圆柱诱导CH4/空气预混燃烧流场。采用保自由流5阶WENO格式求解贴体坐标变换后的多组分Euler方程,用基元反应模型描述CH4/空气燃烧。不同于标准WENO格式通量构造方法,该WENO格式数值通量由方程的解进行WENO插值得到,在曲线坐标系下具有保自由流性质。首先给出了保自由流WENO格式精度和保自由流的数值验证,然后计算圆柱诱导CH4/空气预混气燃烧流场,并考察不同半径圆柱的影响,给出燃烧流场压力与温度等值线和云图、压力和温度沿过驻点线分布。结果表明:在考核计算结果网格无关性基础上,该WENO格式可准确地捕捉激波和火焰阵面形状、激波和火焰面驻点距离,得到的计算结果和文献结果相符。增大圆柱半径,激波和火焰面被推向来流方向,激波和火焰面之间距离也减小。和TVD格式相比,5阶WENO格式采用四分之一的网格数可得到近似相同的计算结果。     

正弦波型高频动态压力光学校准系统及其应用

动态压力是气动部件表面的关键气动参数。光学压力敏感涂料（PSP）测量技术在测量气动部件表面动态压力方面具有全域测量、不影响流场自身的优势，而光学压力敏感涂料的动态响应特性则是进行动态压力测量的决定性因素。基于声学驻波管原理，自主设计并组建了正弦波型高频动态压力光学校准系统，主要包含有驻波管型校准舱、声源、激光源、高频压力传感器、光电倍增管以及测控系统。对动态压力光学校准系统及某新型快响压敏涂料的实验结果表明，所组建的动态压力校准系统可产生最短响应时间12.5 μs、最大压力幅值为4.37 kPa的正弦型动态压力，其有效动态频响范围为0.4~20.0 kHz（50 μs~2.5 ms），不确定度小于0.004 9%；校准系统合理的光路布局可进行快响压敏涂料动态特性的校准，所测涂料可用于动态频响不高于9.1 kHz（响应时间为109.9 μs）的非定常流场的压力测量。     

压力波对垂直管低温气液掺混冷凝的影响

为了分析高压补燃液氧煤油发动机氧泵间管内气液两相掺混冷凝及其压力波传播过程,建立了可产生压力扰动的垂直管低温气液两相掺混实验系统,以氧气/液氧为实验工质,开展压力波对垂直管内低温气液两相掺混冷凝的影响研究,获得了不同压力波频率和氧气流量工况下的掺混图像,分析结果表明:压力波会使发散流型由微弱振荡冷凝向间歇振荡冷凝转变,使椭圆流型由稳定冷凝向振荡冷凝转变;在0~52 Hz不同频率压力波作用下,发散流型最大轴向冷凝长度与掺混孔径之比在10~30之间,椭圆流型的比值在8~15之间变化;压力波对气相摆动频率起主导性和正相关性的影响。     

An optimal beam alignment method for large-scale distributed space surveillance radar system

Large-scale distributed space surveillance radar is a very important ground-based equipment to maintain a complete catalogue for Low Earth Orbit (LEO) space debris. However, due to the thousands of kilometers distance between each sites of the distributed radar system, how to optimally implement the Transmitting/Receiving (T/R) beams alignment in a great space using the narrow beam, which proposed a special and considerable technical challenge in the space surveillance area. According to the common coordinate transformation model and the radar beam space model, we presented a two dimensional projection algorithm for T/R beam using the direction angles, which could visually describe and assess the beam alignment performance. Subsequently, the optimal mathematical models for the orientation angle of the antenna array, the site location and the T/R beam coverage are constructed, and also the beam alignment parameters are precisely solved. At last, we conducted the optimal beam alignment experiments base on the site parameters of Air Force Space Surveillance System (AFSSS). The simulation results demonstrate the correctness and effectiveness of our novel method, which can significantly stimulate the construction for the LEO space debris surveillance equipment.