基于海杂波对消技术的无线电引信超低空技术研究

无线电引信超低空性能实现的关键就是抑制海杂波,提取出目标信号.目前常用的距离波门截止技术和频谱识别技术所能达到的超低空性能还分别有其不足之处.文中针对以上两种技术的缺点,从海杂波对消的角度出发,提出了一种简单而有效的海杂波抑制方法.     

基于RDSS辅助的Doppler/SINS组合导航系统研究

Doppler/SINS组合导航系统具有输出水平速度误差较小、平台角误差较小的优点 ,但存在经纬度误差较大的缺点 ,故不能作为独立的导航定位系统 ;而双星定位系统(RDSS)可输出较高精度的经纬度信息 ,但存在定位滞后的缺陷。利用Doppler/SINS的输出水平速度可以补偿RDSS的位置滞后 ,同时经过位置补偿后的RDSS系统可实时修正Doppler/SINS组合导航系统。仿真结果表明 ,基于RDSS辅助的Doppler/SINS组合导航系统能有效地克服Doppler/SINS系统的缺点 ,是一种新型的组合导航系统 ,可应用于导航定位精度要求较高的场合     

星载合成孔径雷达的一种新波形及其处理技术

分析研究了步进频率脉冲串信号在星载合成孔径雷达 (SAR)中应用时的多普勒效应 ,并提出了一种纵向距离合成高分辨成像时多普勒二次相位的补偿方法 ,从而消除了纵向距离分辨率的恶化和信噪比损失 ,同时还可以消除纵向距离向与方位向之间的多普勒耦合     

电离层不规则结构的多普勒谱特性

利用武汉电离层观象台连续5年的高频多普勒记录,研究电离层中不规则结构反射回波的各种频谱特性及其变化。通常,扩展F回波总是引起扩散的多普勒诺;而Es回波的多普勒图白天一般呈平直光滑谱,晚上变得扩散,其多普勒展宽常比未扩散时大2-3倍,达1Hz以上。多普勒图上有时会出现斜描迹多普勒谱,这种谱结构反映了Es或扩展F中电子云团的漂移运动。      

多卜勒波束锐化运动补偿方法的研究

载机在空中的任何机动行为都会使多卜勒波束锐化(ＤＢＳ)性能下降,严重时甚至失效。针对ＤＢＳ工作特点,对所需的运动补偿方法,进行了深入的分析与研究,给出了运动补偿的一般方法,同时还提出了一种新的用载机在雷达视线(ＬＯＳ)上的投影速度来实时控制脉冲重复周期(ＰＲＦ)的相位补偿方法,并对该方法的精度及其对惯导系统(ＩＮＳ)的容差范围作了分析。最后给出了模拟结果。     

恒速直线连续面扫描激光多普勒测振方法

介绍了一种恒速直线面扫描方式下的连续扫描激光多普勒测振(Continuous scanning laser Doppler vibrometry,CSLDV)方法。该方法在扫描多普勒测振系统的基础上,通过控制激光头两个相互垂直的扫描镜连续恒速运动实现激光点在被测平面连续扫描测试。本文阐述了恒速直线面扫描连续激光多普勒测振的基本理论,以及测试信号处理过程中的延迟去除和振型解调中的滤波器选择、坐标变换等内容,并以平板结构为例完成了连续激光多普勒测振实验及数据分析方法的验证,采用最小化虚部振型的方法解调了测试工作变形。结果表明,由恒速直线面扫描测试获得的工作变形与相应模态振型十分接近,可以作为空间分辨率很高的振型测试数据。连续扫描激光多普勒测振技术是一种高分辨率振型测试的高效方法,具有十分重要的应用价值。     

利用多普勒测量确定嫦娥四号着陆器精密定轨

针对嫦娥四号着陆器环月飞行阶段的轨道，开展基于多普勒测量数据的精密轨道计算与精度分析。首先给出了多普勒测量数据的精确观测建模方法。然后，从着陆器姿控力影响，重叠弧段轨道比较，以及独立轨道比较几个方面开展计算与分析，结果表明：姿控喷气会对探测器产生细微的加速度，对轨道计算产生20~50 m的影响；通过重叠弧段的比较，稳定飞行阶段多普勒数据独立解算轨道的精度优于30 m；与测距与VLBI测量联合解算轨道的比较，轨道之间的差异小于50 m。     

Using cross correlation to estimate Doppler frequency

Doppler frequency estimation with high accuracy is very important for precise orbit determination and scientific studies in deep space exploration. In this paper, we propose a new method which implements cross correlation of only received signals from one single station to estimate Doppler frequency. The algorithm is relatively simple and it can achieve high accuracy even when signal to noise ratio (SNR) is very low. Moreover, the accuracy can be further improved by implementing frequency compensation, especially when the frequency dynamic range is high. Simulations were performed and results proved the validity of this method. X-band observations on MEX (Mars Express) and Juno were performed by a 13 m telescope of Wuhan University, which was equipped by two back ends, i.e. CDAS (Chinese Data Acquisition System) and RSR (Radio Science Receiver). Raw data recorded by the CDAS were processed by using the proposed method, and the estimated frequencies were in good agreement with the real time frequency estimation values by the RSR. What’s more, the accuracy by using cross correlation was higher than the one of RSR.     

高扰动燃油喷嘴雾化试验

为改善航空发动机的燃油雾化、验证高扰动雾化方案应用于航空发动机燃油喷射的可行性,采用相位多普勒粒子分析仪(PDPA)及高速摄影技术,对不同夹角、不同孔径结构条件下的V形交叉孔高扰动喷嘴和单孔喷嘴的喷雾场粒子特性进行了测量。结果表明:随着供油压差增大,雾化锥角随之增大,索太尔平均直径(SMD)值随之减小;交叉孔结构对燃油雾化有明显促进作用,在相同的供油压差、出口截面积条件下,交叉孔的雾化锥角更大,SMD更小;在SMD相同时,交叉孔所需的喷射压力远小于圆直孔;随着交叉角的增加,雾化锥角、SMD均有明显改善;采用空气辅助能够有效增大雾化锥角、降低SMD值,但改善效果随气压增加而逐渐减弱。与传统单孔喷孔方案相比,高扰动喷孔能够在相同压力条件下极大的改善燃油雾化效果。      

Integral inversion of GRAIL inter-satellite gravitational accelerations for regional recovery of the lunar gravitational field

We present an integral-based approach for high-resolution regional recovery of the gravitational field in this article. We derive rigorous remove-compute-restore integral estimators relating the line-of-sight gravitational acceleration to an arbitrary order radial derivative of the gravitational potential. The integral estimators are composed of three terms, i.e., the truncated integration, the low-frequency line-of-sight gravitational acceleration, and the high-frequency truncation error (effect of the distant zones). We test the accuracy of the integral transformations and of the integral estimators in a closed-loop simulation over the Montes Jura region on the nearside of the Moon. In this way, we determine optimal sizes of integration radii and grid discretisation. In addition, we investigate the performance of the regional integral inversion with synthetic and realistic GRAIL observations. We demonstrate that the regional inversion results of the disturbing gravitational potential and its first order radial derivative in the Montes Jura mountain range are less contaminated by high-frequency noise than the global spherical harmonic models.