瞄准指示器光路设计

介绍了瞄准指示器的光路设计原理，着重讲述分光镜的设计原理，并对干涉场光强分希进行了简单推导，给出了瞄准测量的判断依据。     

用相位偏移干涉法精确测量量块长度

讨论了相位偏移干涉技术的原理、常用的算法和小数重合法的应用。在分析了传统的柯氏干涉仪的量块测量方法基础上 ,提出运用相位偏移干涉法的量块测量法 ,最后给出了量块测量的数据。     

湍流流场双向全息干涉测量

多方向全息干涉法是获得三维流场重构数据的较好方法,采用离轴式像面全息干涉技术从正交两方向对同一流场进行显示,得到了模型流场清晰的序列全息干涉图,可用于三维重构数据提取的需要。同时,采用CFI仿真结果进行对比验证。通过对该研究的总结和分析,为今后多向（≥6方向）全息干涉技术测量湍流流场奠定了基础,同时也提出了下一步工作的相关想法。     

全息测振干涉图的自动分析与处理

 研究数字条纹图象的自动检测与判读处理的理论与技术,在微型通用数字图象处理系统上建立了一套条纹自动检测与判读处理的软系统,实现了条纹图象的输入、定位、预处理、骨架化、细化、修补与光滑、计数、插值及三维振幅场输出等功能,对类似的散斑干涉条纹和莫尔条纹的判读处理有理论参考价值。     

Space very long baseline interferometry in China

Space very long baseline interferometry (VLBI) has unique applications in high-resolution imaging of the fine structure of astronomical objects and high-precision astrometry due to the key long space–Earth or space–space baselines beyond the Earth’s diameter. China has been actively involved in the development of space VLBI in recent years. This review briefly summarizes China’s research progress in space VLBI and the future development plan.     

Data processing center of RadioAstron space VLBI project

In this paper, questions on development, implementation, and operation of RadioAstron project Data Processing Center (DPC) are reviewed. The main components of the dedicated DPC are the computer complex with 1 TFlops/s performance, storage with memory capacity of approximately 10 PB, the network infrastructure, and the corresponding communication channels. Performance enhancement methods and resolution of information storage, archiving, and process problems of space VLBI high-speed digital data flows are analyzed. It is shown that successful operation of DPC is mainly provided by optimal organization of computer system structure, storage, and networking transmission. Some of the important key features of RadioAstron project DPC and its comparative differences from the standard VLBI procedures are considered.     

Technology challenges for space interferometry: The option of mid-infrared integrated optics

Nulling interferometry is a technique providing high angular resolution which is the core of the space missions Darwin and TPF. The first objective is to reach a deep degree of starlight cancelation in the range 6–20 μm, in order to observe and to characterize the signal from an earth-like planet. Among the numerous technological challenges involved in these missions, the question of the beam combination and wavefront filtering has an important place. A single-mode integrated optics (IO) beam combiner could support both the functions of filtering and the interferometric combination, simplifying the instrumental design. Such a perspective has been explored in this work within the project Integrated Optics for Darwin (IODA), which aims at developing a first IO combiner in the mid-infrared. The solutions reviewed here to manufacture the combiner here are based on infrared dielectric materials on one side, and on metallic conductive waveguides on the other side. With this work, additional inputs are offered to pursue the investigation on mid-infrared photonics devices.     

半导体激光器干涉测距进展

全面评述了近年来半导体激光器应用于干涉测距的进展,对其中的代表性文献进行了详细的分析,指出了该技术今后的主要发展方向和关键问题。     

基于ATI技术和象素匹配的星载SAR/GMTI实现方法

与机载合成孔径雷达相比,星载合成孔径雷达由于其复杂的空间几何关系、地球自转及地球曲率等因素的影响,使得星载SAR／GMTI的实现更为复杂。提出了当不满足相位偏置中心天线(DPCA)中脉冲重复频率和天线水平基线间的严格约束条件时,通过象素匹配法和星载SAR沿航迹向干涉(ATI)技术实现星载合成孔径雷达(SAR)动目标检测、测速及定位的一种方法。该方法采用沿航迹向线性排列的双孔径天线星载SAR结构,首先建立了星载SAR双孔径天线空间几何模型并详细分析了星载SAR双孔径天线机理及信号特性,然后利用常规方法成像的双天线SAR图像,分析并推导了基于ATI技术和象素匹配实现对地面背景杂波淹没的运动目标检测、径向速度分量估计以及目标定位的方法。最后,通过计算机仿真验证了其有效性。