“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.     

信息时代的飞行力学

基于现代信息技术，扼要论述了作为信息时代的飞行力学－－计算飞行力学的产生背景、问题表述、理论框架和计算系统，以及计算飞行力学在未来飞行器发展和运用研究中的作用。     

2021 Turkey mega forest Fires: Biodiversity measurements of the IUCN Red List wildlife mammals in Sentinel-2 based burned areas

Mega wildfires are one of the environmental disasters worldwide. This study evaluates the pre-fire species diversity and the indirect effects, including habitat loss for one of the largest wildfires in Manavgat (Antalya-Turkey) in 2021, with a two-step methodology. Here, (1) burnt areas in the Manavgat district (2021) were detected with remote sensing data from Sentinel-2A by delta Normalized Burn Ratio calculation for a selected area in Google Earth Engine, and (2) mammals' habitat vector data of International Union for Conservation of Nature (IUCN) Red List were integrated into Habitat and Biodiversity modelling of Terrset to analyze the alpha, beta, gamma diversity and Range Restriction Index for the wildfire region. In the total 4210 km² study area, 696 km² of the area was damaged by different fire severity; also, there were 56 mammal species' habitats here. These species include bats (i.e. Nyctalus leisleri), felids (i.e. Felis chaus), rodents (i.e. Rattus norvegicus) and large mammals (i.e. Ursus arctos). 88 % of these species are in IUCN's Least Concern category. The remaining classes are Near Threatened (3.7 %) and Vulnerable (7.4 %). This study also indicated that the burnt area's species richness does not totally consist of endemic species. Therefore, pre-fire species richness analyses of this study can be a base for further studies about the species' post-fire activity and occupancy.Furthermore, the 2021 mega wildfires show us the necessity of wildfire monitoring and risk studies in the entire Mediterranean ecosystem to evaluate the risks to the Sustainable Development Goals. Therefore, post-fire spatial data, fire migration monitorization, and recording of the species' activities should be performed temporally. In this way, the ability of wildlife's recovering, and the direct and indirect effects of the fire will be examined for ecosystems in the long term.     

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。     

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.     

模糊传感器与区间型多属性决策的信息融合方法

对于日益复杂的信息环境和变化的目标特性,现有的多传感器信息融合方法大多为"静态的",较少考虑传感器可信度变化以及测量过程中的多维特征指标权重的时效性给融合结果带来的影响.为了解决此问题,提出了一种基于模糊理论与区间型多属性决策的信息融合方法.该方法从各传感器对模糊命题支持度的一致性来定义其信息质最优化度,用区间数与多属性决策理论来定义特征识别综合置信度,并从这两方面客观确定了传感器的融合权重,较好地解决了对传感器信息与目标特征权重为模糊与不确定时的合理评价,以此构建了一个智能优化决策层融合识别模型.最后以弹道目标识别实验证明了此方法有较好的时效性和准确性.     

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。     

一种新的辐射源优化识别方法

针对证据理论无法获得传感器报告、无法处理具有冲突的传感器报告、计算复杂度高、干扰环境下融合结果不可靠等缺点,提出了一种新的辐射源优化识别方法。该方法首先利用灰色关联算法来获得传感器的报告,并且提出利用信息熵解决灰色关联分析中特征权重的选择问题。然后根据传感器证据报告的特点,引入传感器可信度因子,通过构造和分解代价函数将辐射源识别问题转化为求解一个凸二次优化问题。最后,给出了一种利用对数罚函数方法求解该问题的改进方法和步骤。理论分析和仿真结果表明,与证据理论相比,新方法具有更低的计算复杂度、更好的识别能力、更广的适用性和更强的鲁棒性。
     

Removing orbital debris with lasers

Orbital debris in low Earth orbit (LEO) are now sufficiently dense that the use of LEO space is threatened by runaway collision cascading. A problem predicted more than thirty years ago, the threat from debris larger than about 1 cm demands serious attention. A promising proposed solution uses a high power pulsed laser system on the Earth to make plasma jets on the objects, slowing them slightly, and causing them to re-enter and burn up in the atmosphere. In this paper, we reassess this approach in light of recent advances in low-cost, light-weight modular design for large mirrors, calculations of laser-induced orbit changes and in design of repetitive, multi-kilojoules lasers, that build on inertial fusion research. These advances now suggest that laser orbital debris removal (LODR) is the most cost-effective way to mitigate the debris problem. No other solutions have been proposed that address the whole problem of large and small debris. A LODR system will have multiple uses beyond debris removal. International cooperation will be essential for building and operating such a system.