THREE ASPECTS OF ISAR SIGNAL PROCESSING

ＴＨＲＥＥＡＳＰＥＣＴＳＯＦＩＳＡＲＳＩＧＮＡＬＰＲＯＣＥＳＳＩＮＧＳｈｅＺｈｉｓｈｕｎ；ＺｈｕＺｈａｏｄａ（ＤｅｐａｒｔｍｅｎｔｏｆＥｌｅｃｔｒｏｎｉｃＥｎｇｉｎｅｅｒｉｎｇ，ＮＵＡＡ２９ＹｕｄａｏＳｔｒｅｅｔ，Ｎａｎｊｉｎｇ２１００１６Ｐ．Ｒ．Ｃ...     

考虑电离层对GEOSAR影响的改进CS成像算法

地球同步轨道合成孔径雷达(GEOSAR)轨道位置高且合成孔径时间较长,电离层的空时变化特性严重影响该雷达的聚焦性能。为解决电离层对GEOSAR成像聚焦性能的影响,提出一种改进的chirp scaling (CS)成像算法。结合GEOSAR的轨道运动特点,给出因电离层空时变化引起的回波信号模型,提出了改进CS成像算法用以解决电离层对成像聚焦性能的影响。仿真结果表明:该成像方法能较好地处理电离层影响,可获得理想的聚焦成像结果。该方法为GEOSAR实现高精度成像提供了技术支撑。     

现代飞机尾旋平衡点的分析和预测

 本文提出了两种近似估计稳态尾旋平衡点的方法。一种是通过忽略一些对稳态尾旋影响不大的参数,理论上得出了稳态尾旋时各量的近似值;另一种方法是通过计算机,运用最优化方法——DFP变尺度法,算出平衡点的值,从而大大缩短了尾旋运动的数字仿真时间,为改进尾旋的研究提供了方便。     

地基雷达探测方位对目标识别的影响研究

导弹防御系统的地基X波段雷达和海基X波段雷达是进行目标识别的主要传感器,它们只有在探测到目标以后才能通过记录目标的相关特性,进行目标识别。由于雷达探测的方向不同,探测到的目标散射截面也不同,因此,在导弹突防过程中,可通过调整弹头的飞行姿态,改变雷达探测方位,从而最大限度地减小目标散射截面,最终影响雷达识别目标的效果。     

Improvements in bottomside electron density definition in the Autoscala program

Some improvements introduced in the Autoscala program are presented. They include improvements in E valley modeling of the electron density profile N_e(h), and in the link between the E valley and bottom-side F regions. An abrupt variation in N_e(h) generated by the previous version of Autoscala under night conditions has been eliminated.A series of ionograms recorded by the Millstone Hill digisonde (42.6°, 288.5°) were automatically interpreted by the previous version of Autoscala and by the new one. Data from Incoherent Scatter Radar (ISR) were used to comparatively assess the performance of the two versions. For this purpose, the root mean square errors (RMSEs) of the N_e(h) provided by Autoscala were calculated relative to the corresponding values provided by ISR.A more accurate overall modeling of N_e(h) was achieved by the new Autoscala version (RMSE = 0.51 MHz for the new version against RMSE = 0.67 MHz for the previous one).     

基于LFT的鲁棒变增益控制的降保守性设计

研究了线性变参数系统的鲁棒变增益控制,介绍了基于LFT的鲁棒变增益控制的思想;针对目前基于LFT的鲁棒变增益控制的保守性,采用全块标量矩阵,通过减少对全块标量矩阵的结构约束;提出了一种保守性更小的稳定性判据,并且利用消元定理,给出了基于LFT的鲁棒变增益的输出反馈控制器存在的条件;同时给出了控制器的构建方式,并且给出了...     

中继卫星星间天线指向误差传播率研究

基于中继卫星星间天线对用户航天器的跟踪规律,建立了准确的误差传递模型,并对分析结果进行了仿真验证。文中首先定义了误差传递模型所需的各类坐标系;然后使用微分方法分别建立了中继卫星轨道误差传递模型、中继卫星姿态误差传递模型,分析了滚动角、俯仰角和偏航角与指向精度之间的关系,以及位置保持控制对指向精度的影响;最后借助于STK软件的轨道计算功能,使用蒙特卡罗方法进行数学仿真,仿真结果验证了误差传递模型的准确性。     

Towards Synthesis of Solar Wind and Geomagnetic Scaling Exponents: A Fractional Lévy Motion Model

Mandelbrot introduced the concept of fractals to describe the non-Euclidean shape of many aspects of the natural world. In the time series context, he proposed the use of fractional Brownian motion (fBm) to model non-negligible temporal persistence, the ‘Joseph Effect’; and Lévy flights to quantify large discontinuities, the ‘Noah Effect’. In space physics, both effects are manifested in the intermittency and long-range correlation which are by now well-established features of geomagnetic indices and their solar wind drivers. In order to capture and quantify the Noah and Joseph effects in one compact model, we propose the application of the ‘bridging’ fractional Lévy motion (fLm) to space physics. We perform an initial evaluation of some previous scaling results in this paradigm, and show how fLm can model the previously observed exponents. We suggest some new directions for the future.     

发射点定位误差对发射方位角的影响

发射点定位误差对发射坐标系的影响不仅仅在于坐标系原点不准，而且还会影响发射方位角，从而会有欧拉角的转换。首先依据确定平面的几何原理和求解平面夹角的余弦公式，在地心坐标系下，得到发射方位角与发射点、目标点的简洁的解析关系；然后，通过地心坐标系为中介推导了发射坐标系的扰动矩阵。由此，可得到发射点经度、纬度和高程的变化对发射方位角影响的量化结论。