星载成像雷达运动补偿

本文分析了星载成像雷达的误差来源,运动误差产生的影响,对各种运动补偿方法进行了理论分析和比较.     

调频引信谐波时序检测抗干扰方法及实现

针对调频（FM）引信抗干扰能力差的问题,提出了调频引信谐波时序检测抗干扰方法,利用弹目交会过程中谐波时序特征,提高了调频引信抗调幅（AM）、调频和扫频干扰能力;设计了基于快速傅里叶变换（FFT）的调频引信谐波提取方案,通过对差频信号进行FFT获得谐波幅值,与现有谐波定距调频引信通过带通滤波器（BPF）获得谐波幅值相比,在保证同等定距精度的前提下,可以灵活选取谐波次数和谐波通道,利用谐波时序性提高调频引信抗干扰能力,同时易于实现炸高分挡。仿真及实测结果验证了本文方案的可行性,调频引信抗干扰成功率由16.7%提高到90%以上。      

激光测速技术（LDV）诞生50周年启示

回顾50年来激光测速技术（LDV）的发展过程,取得的主要成就,科学家和工程技术人员作出的重大贡献。LDV为流体力学的实验研究提供了有力的测试手段,开辟了对复杂流动精确、定量、动态测量研究的新篇章。     

一种高动态低信噪比下载波快速捕获跟踪方法

针对高动态、低信噪比的接收信号,首先对整个多普勒频率范围进行分段,并在每一段内利用本地产生的带有多普勒频率变化率的复信号来抵消接收信号中多普勒频率变化率的影响,然后在每一段内利用FFT（FastFourierTransform,快速傅里叶变换）进行载波频率并行捕获,从而同时完成载波多普勒频率及其变化率的初步估计。利用载波多普勒频率及其变化率估计信息辅助锁频环快速入锁,进而利用锁频环辅助三阶锁相环完成载波信号的锁频锁相跟踪。使用这种方法,可以快速获取信号的多普勒频率及其变化率信息,并且在极短时间内完成载波的稳定跟踪,使接收设备具备快速捕获跟踪大动态弱信号的能力。     

旋转方截面U型通道分离流二阶相关分量测量

为了深入了解旋转涡轮叶片内冷通道中的紊流特性，并为CFD研究提供实验数据，用激光多普勒测速仪（LDA）测量了旋转U型通道中分离流的雷诺应力分量。通道的转轴与弯道的曲率轴平行，测量是在与转轴垂直的对称平面中进行的，流动状态为Re=100,000,Ro=0,0.2和－0．2。直接测量的分量为ux^2^-,Ux^2^-和uxux^-，结果表明旋转对紊流分布的形式有很强的影响。在测量的三种旋转状态中Ro=0.2的正转和Ro=0.2的负转分别具有最低和最高的紊流强度。根据测量到的信息估算了雷诺应力uiuj^-的产生率，结果显示负转的产生率比正转时高。     

大斜视直升机载太赫兹ViSAR振动补偿成像算法

太赫兹视频合成孔径雷达（ViSAR）载波波长短,直升机载平台的微小高频振动将引起回波信号相位的显著变化,进而严重恶化ViSAR的成像性能。本文在建立斜视ViSAR平台振动成像几何模型的基础上,提出了大斜视模式下的振动相位误差补偿成像算法。该算法结合运动补偿原理,将斜视成像侧视化处理,然后采用改进的多普勒Keystone变换方法在二维频域校正由平台振动引起的距离单元徙动,最终在距离多普勒域实现振动相位误差补偿。仿真结果验证了该算法的有效性。      

机载双天线前视SAR系统成像分析

针对机载SAR前视模式与一般正侧视模式存在的明显不同,详细分析了前视SAR的多普勒特性及其方位模糊问题.依据前视SAR的特性,结合波束锐化与RD成像算法,仿真得到了前视SAR的点目标图像,验证了分析的正确性.     

A novel range-Doppler imaging algorithm with OFDM radar

Traditional pulse Doppler radar estimates the Doppler frequency by taking advantage of Doppler modulation over different pulses and usually it requires a few pulses to estimate the Doppler frequency. In this paper, a novel range-Doppler imaging algorithm based on single pulse with orthogonal frequency division multiplexing(OFDM) radar is proposed, where the OFDM pulse is composed of phase coded symbols. The Doppler frequency is estimated using one single pulse by utilizing Doppler modulation over different symbols, which remarkably increases the data update rate. Besides, it is shown that the range and Doppler estimations are completely independent and the well-known range-Doppler coupling effect does not exist. The effects of target movement on the performances of the proposed algorithm are also discussed and the results show that the algorithm is not sensitive to velocity. Performances of the proposed algorithm as well as comparisons with other range-Doppler algorithms are demonstrated via simulation experiments.     

Supertyphoon Hagibis action in the ionosphere on 6–13 October 2019: Results from multi-frequency multiple path sounding at oblique incidence

The purpose of the present paper is to describe the observations of the variations in the parameters of HF radio waves propagating through the ionosphere when the action of the super typhoon Hagibis on 6–13 October 2019 occurred. The observations have been made with the Harbin Engineering University (the People's Republic of China) multi-frequency multiple path radio system involving the software-defined technology. The action of the super typhoon has been shown to be accompanied by enhanced atmospheric wave activity acting to generate wave processes with periods of 10 to 120 min. Coupling in the atmosphere–upper-atmosphere–ionosphere system has been confirmed to be carried out with atmospheric gravity waves. The ionosphere underwent the greatest impact on those days when the supertyphoon had maximum energy, on 8, 10, and especially 9 October 2019, and when it was found to be in an ～2,500–3,000-km distance range from the propagation path midpoints. Under the action of wave processes, the height of the reflection region was observed to oscillate within the ±(30–90 km) limits. The amplitude of the quasi-periodic variations in the ionospheric F-region electron density was estimated to be 10–12% for periods of ～20 min, and 30–60% for periods of ～60–120 min. The joint action of the dusk terminator and the supertyphoon has been confirmed to enhance wave activity in the ionosphere. Similar effects for the dawn terminator have not been detected.