一种高斯型ASE光源研究

简单介绍了掺铒光纤的光放大原理,分析了四种ASE光源的光路结构。针对双通前向结构,设计了一种适用高精度光纤陀螺仪的高斯型ASE光源,并进行了试验研究。试验结果表明,掺铒光纤的掺杂浓度、光纤长度都对ASE光源的输出特性具有很大的影响。此外,根据试验结论,研制出高斯型ASE光源,其性能稳定,已在多个高精度光纤陀螺仪型号上实现了实际应用,并取得了良好的效果。     

跨声速流自发凝结水滴的测量

应用基于多波长消光法原理发展的光学探针,测量了跨声速风洞中不同马赫数湿空气流自发凝结形成的水滴尺寸及浓度,并给出了实验结果     

光标产生器和液晶眼镜光电同步驱动器

论述了时分式立体电视系统中光标产生器和液晶眼镜光电同步驱动器的工作原理和功能，并设计出具体的实用电路     

透光脉动值在絮凝实验研究中的应用

通过理论分析和实验研究，以流动原水为研究对象，首次考察了PAM、PAC、PAF和PFS几种絮凝剂在絮凝过程中的透光脉动值变化。结果表明，不同种类絮凝剂投加条件下所形成的絮凝体具有不同的特性，能及时得到絮凝体破碎和重组的有关信息。     

空间流场显示的一种新方法──激光片光运动法

用一套能在气垫滑轨上平稳运动的激光片光运动系统，对湍流边界层及其拟序结构进行了空间流场显示，并对其应用范围、使用方法和技术等进行了研究。实验结果表明，这种空间显示法不仅能够较好地揭示流场的空间结构，而且与其它空间流场显示法相比，具有费用低，操作方便，应用范围较广，易于对照片进行准确的定量分析等优点。     

大型运输机动力增升喷流效应数值模拟

参照C-17运输机发动机安装位置,考虑内、外涵道分开排气,建立了外吹式襟翼动力增升全机几何分析模型以及相应的巡航构型.采用结构化多块网格技术,基于雷诺平均Navier-Stokes方法,分别对全机增升构型和单独发动机动力喷流进行数值模拟验证,在此基础上对外吹式襟翼动力喷流效应展开研究.对于低速动力增升构型,发动机喷流大部分直接冲刷襟翼下表面而后向下偏转,部分高速气流经襟翼缝道引射并加速后吹向襟翼上表面,两部分气流在襟翼后缘汇合并向下游延伸,喷流冲刷襟翼时存在明显展向横流特征.在动力喷流影响下,不仅襟翼环量大幅增加,缝翼和主翼上的环量也均有所增加,全机可用升力系数和最大升力系数均突破了机械式增升装置的极限,达到4.0以上.同时,全机低头力矩大幅增加,为纵向配平带来额外的压力.对于相应的高速巡航构型,发动机喷流主要影响机翼下表面的压力分布,使得全机升力减小,阻力明显增大.动力增升构型在基本翼设计过程中应充分考虑喷流的影响.      

基于ICCD的空间微光成像系统成像性能研究

研究基于像增强型CCD（ICCD）的空间高分辨率微光成像系统的成像性能。通过理论推导及数学仿真的方法，对系统在微光条件下的能量传递、极限分辨力、信噪比以及调制传递函数进行分析计算。研究表明，系统在黎明照度条件下具有较好探测能力，通过对ICCD器件制冷可以有效提高系统信噪比，实现满月照度的探测成像。     

红外辐射测量系统内部杂散辐射建模与仿真

杂散辐射是影响光学系统性能的重要因素,对于红外光学系统,除了外部杂散辐射,还须考虑系统自身结构产生的内部杂散辐射。为提高红外辐射计内部杂散辐射分析的精度,建立了 1种基于复合蒙特卡洛法的内部杂散辐射数学模型。首先,将红外辐射计的内部杂散辐射源根据位置分为 2部分:遮光罩入瞳处的热辐射和辐射计内部光学元件、机械部分所发出的热辐射。对于遮光罩入瞳处和辐射计内部光机元件发出的杂散辐射,分别采用正向蒙特卡洛法和反向蒙特卡洛法进行追踪,得到探测器接收面入瞳处的杂散辐射辐照度分布,进而分析不同位置的发射源对接收面入瞳处的杂散辐射贡献。最后,与直接模拟仿真结果进行对比。实验结果表明,在追迹光线数相等的情况下,该方法的精度更高。仿真结果体现了红外辐射计各部分杂散辐射对探测器入瞳面接收到的杂散辐射造成的影响,对后期开展内部杂散辐射抑制提供了方向。     

Scientific requirements for future spatially resolved white-light and broad-band high-cadence observations of the Sun

Several important issues are open in the field of solar variability and they wait their solution which up to now was attempted using critical ground-based instrumentations. However, accurate photometric data are attainable only from space. New observational material should be collected with high enough spatial and spectral resolution, covering the whole visible range of the electromagnetic spectrum as well infrared and ultraviolet to reconstruct the total solar irradiance: (1) the absolute contributions of different small-scale structural entities of the solar atmosphere from the white light flares and from micro-flares are still poorly known; (2) we do not know the absolute contributions of different structural elements of the solar atmosphere to the long-term and to the cyclic variations of the solar irradiance, including features of the polar regions of the Sun; (3) the variations of the chromospheric magnetic network are still poorly evaluated; (4) only scarce information is available about the spectral variations of different small-scale features in the high photosphere. Variability of the Sun in white light can be studied with higher spectral, spatial and time resolution using space-born telescopes, which are more appropriate for this purpose than ground based observatories because of better seeing conditions, no interference of the terrestrial atmosphere and a more precise calibration procedure. Scientific requirements for such observations and the possible experimental tools proposed for their solution. Suggested solar studies have broader astrophysical importance.     

Three-line structured light vision system for non-cooperative satellites in proximity operations

Adapter ring is a commonly used component in non-cooperative satellites, which has high strength and is suitable to be recognized and grasped by the space manipulator. During proximity operations, this circle feature may be occluded by the robot arm or limited field of view. Moreover, the captured images may be underexposed when there is not enough illumination. To address these problems, this paper presents a structured light vision system with three line lasers and a monocular camera. The lasers project lines onto the surface of the satellite, and six break points are formed along both sides of the adapter ring. A closed-form solution for real-time pose estimation is given using these break points. Then, a virtual structured light platform is constructed to simulate synthetic images of the target satellite. Compared with the predefined camera parameters and relative positions, the proposed method is demonstrated to be more effective, especially at a close distance. Besides, a physical space verification system is set up to prove the effectiveness and robustness of our method under different light conditions. Experimental results indicate that it is a practical and effective method for the pose measurement of on-orbit tasks.