星间光通信中BER的口径自适应控制法

从接收机的比特误码率与发射机的振动关系出发,采用OOK调制方式,以APD为光电探测器,推导得到了描述发射机天线口径与发射机振动关系的数学模型。针对比特误码率(BER)随振动幅值增加而上升的问题,提出了用发射天线口径与自适应方法控制BER的解决方案。用MATLAB6.5计算得到了自适应和标准条件下BER与跟踪系统信噪比的关系曲线。计算结果表明,采用天线口径自适应方法可将BER值控制在设计要求以下。     

空间卫星红外辐射灵敏度分析

考虑卫星本体表面包覆绝热材料的实际物理状态,根据数值传热学和有限容积法建立了目标表面温度场和红外辐射计算模型.建立卫星结构模型,基于热控涂层性能退化,提出红外辐射灵敏度概念,并建立了卫星红外辐射灵敏度计算模型.对在轨飞行卫星的瞬态温度场进行数值模拟,与遥测数据对比分析.最后,分析了空间卫星的红外辐射和红外辐射灵敏度.结...     

共形光学系统设计研究

共形光学整流罩在保证了光学指标的前提下,与后端的其他结构外形轮廓平滑连接,从而提高了飞行器空气动力学的性能,在航空航天领域具有重要的应用价值。然而,采用特殊面型的整流罩给共形光学系统的像差校正以及加工、检测方面带来了极大的挑战。本文首先分析了共形整流罩像差特性,并在此基础上介绍了两种典型的光学设计。     

“自准”赝像及识别

置平面镜于凸透镜后,则凸透镜前焦平面上的物成像于该物平面上,即“自准”成像.满足其它条件也能成像于物平面.分析不同条件下像的形成及其特点,并给出识别自准成像的判据.     

Computational engineering analysis of external geometrical modifications on MQ-1 unmanned combat aerial vehicle

This paper focuses on the effects of external geometrical modifications on the aerodynamic characteristics of the MQ-1 predator Unmanned Combat Aerial Vehicle (UCAV) using computational fluid dynamics. The investigations are performed for 16 flight conditions at an altitude of 7.6 km and at a constant speed of 56.32 m/s. Two models are analysed, namely the baseline model and the model with external geometrical modifications installed on it. Both the models are investigated for various angles of attack from −4° to 16°, angles of bank from 0° to 6° and angles of yaw from 0° to 4°. Due to the unavailability of any experimental (wind tunnel or flight test) data for this UCAV in the literature, a thorough verification of calculations process is presented to demonstrate confidence level in the numerical simulations. The analysis quantifies the loss of lift and increase in drag for the modified version of the MQ-1 predator UCAV along with the identification of stall conditions. Local improvement (in drag) of up to 96% has been obtained by relocating external modifications, whereas global drag force reduction of roughly 0.5% is observed. The effects of external geometrical modifications on the control surfaces indicate the blanking phenomenon and reduction in forces on the control surfaces that can reduce the aerodynamic performance of the UCAV.     

自适应光学技术补偿镜面温度及自重变形研究

论述了在星载高分辨率相机上采用自适应光学技术的必要性;介绍了应用自适应光学技术补偿镜面温度及自重变形的实验原理,进行了计算机模拟计算,并与实验结果进行比较。实验用一块平面反射镜作为缩比模型,应用６１单元自适应光学系统对其进行了闭环校正实验,分析了泽尼克多项式所对应的像差的校正效果。     

一种融合MRF分割与数学形态学的道路提取算法

针对高分辨率合成孔径雷达（Synthetic Aperture Radar, SAR）图像中道路目标难以有效提取的问题,提出一种融合马尔可夫随机场（Markov Random Field, MRF）分割与数学形态学处理的高分辨率SAR图像道路提取算法。该算法首先利用直方图均衡化和增强Lee滤波对SAR图像进行预处理,实现道路的边缘增强,抑制相干斑噪声;进而利用基于条件迭代模式（Iterated Conditional Mode, ICM）的MRF对SAR图像中的道路目标进行初分割;再用数学形态学填充空洞,平滑道路边缘;最后,基于道路的几何特征,使用偏心率、矩阵度、复杂度等因子去除虚警,从而提取出道路目标。利用该文算法对两块实际高分辨率SAR图像进行道路目标提取,均可以取得90%以上的正确道路提取率,表明本文算法具有较高的道路提取精度。     

高超声速条件下星光传输模拟方法与仿真

以高超声速飞行器为研究对象,建立了高速流场下的星光传输模拟仿真方法,定性、定量地研究平台气动光学效应对星光导航的影响。采用基于k-ω/SST两方程湍流模型的雷诺平均法计算星敏感器安装在飞行器不同位置处（头部、中部和尾部）的外流场密度分布,进而得到流场的空间折射率分布。在此基础上,利用几何光学法计算星光由高速层流流场引起的光程差、点扩散函数、像偏移等光学传输效应,得出经过层流流场的星光降晰图。同时运用统计光学理论计算高速湍流流场引起的星光出瞳面的波像差、密度均方差、相位均方差、Strehl比等光学传输效应,得出经过湍流流场的星光降晰图。仿真结果与理论分析吻合,从而为研究星光在高超声速流场中传输的机理提供了可靠的技术手段。     

Applications of tuned mass dampers to improve performance of large space mirrors

In order for future imaging spacecraft to meet higher resolution imaging capability, it will be necessary to build large space telescopes with primary mirror diameters that range from 10 m to 20 m and do so with nanometer surface accuracy. Due to launch vehicle mass and volume constraints, these mirrors have to be deployable and lightweight, such as segmented mirrors using active optics to correct mirror surfaces with closed loop control. As a part of this work, system identification tests revealed that dynamic disturbances inherent in a laboratory environment are significant enough to degrade the optical performance of the telescope. Research was performed at the Naval Postgraduate School to identify the vibration modes most affecting the optical performance and evaluate different techniques to increase damping of those modes. Based on this work, tuned mass dampers (TMDs) were selected because of their simplicity in implementation and effectiveness in targeting specific modes. The selected damping mechanism was an eddy current damper where the damping and frequency of the damper could be easily changed. System identification of segments was performed to derive TMD specifications. Several configurations of the damper were evaluated, including the number and placement of TMDs, damping constant, and targeted structural modes. The final configuration consisted of two dampers located at the edge of each segment and resulted in 80% reduction in vibrations. The WFE for the system without dampers was 1.5 waves, with one TMD the WFE was 0.9 waves, and with two TMDs the WFE was 0.25 waves. This paper provides details of some of the work done in this area and includes theoretical predictions for optimum damping which were experimentally verified on a large aperture segmented system.     

基于分布式信源编码和感兴趣区域编码的干涉多光谱图像压缩

基于干涉多光谱图像特点和应用环境要求,提出一种基于分布式信源编码和感兴趣区域编码的干涉多光谱图像压缩算法。编码端通过关键帧预测出边信息帧,然后联合估计的边信息帧和插值分布的概率模型在编码端进行比特平面码率估计,最后采用基于率失真提升的感兴趣区域编码,调整图像不同区域的率失真斜率来进行更合理的码率分配。实验结果表明,该算法比传统算法更好地保护了多光谱图像的光谱信息。在不同压缩比的情况下,这种编码方式在干涉多光谱图像压缩系统中可获得较好的效果,算法复杂度低。