电铸镍Wolter I型光学系统制造技术发展综述

摘要： 为满足未来脉冲星导航和空间天文观测任务对X射线望远镜的载荷需求，Wolter I光学系统的研制正逐渐成为新的研究热点，电铸镍方案是当前国内外X射线光学系统镜筒制造的主要技术方案.文章对电铸镍X射线光学系统制造工艺、国内外研制现状、未来应用需求进行了介绍和整理，梳理了电铸镍X射线光学系统研制遇到的关键技术和难点，提出了后续研究发展建议，以促进中国在 X射线脉冲星自主导航、空间探测领域的快速发展.     

万工显滑板移动直线度的检修

通过对影响万能工具显微镜滑板移动直线度的分析 ,提出有针对性的修理方法 ,并分别论述了产生线值偏差和角度偏差的主要原因。     

光敏元件与光传感器的市场动态和发展

介绍了光敏元件与光传感器技术的发展及在国民经济和军事领域中的重要怍用；分析了国内外光电子产业的市场动态与发展趋势；论述了我国光电子产业面临的机遇和挑战。     

振动对空间光通信系统误码率影响的分析

在空间光通信系统中，由于卫星平台的振动，使得光发射机发生振动，从而对通信系统的误码率产生影响，本文针对光射光束为高斯光束时，振动对误码率的影响问题进行研究。结果表明，在振动时不仅振幅影响着误码率，而且波长也对误码率有影响，但通信距离对误码率的影响不大，一般可以忽略。     

A Geosynchronous Orbit Search Strategy

Since more than 10 years there is evidence that small-size space debris is accumulating in the geosynchronous orbit (GEO), probably as the result of breakups. Two break-ups have been reported in GEO. The 1978 break-up of an EKRAN 2 satellite, SSN 10365, was identified in 1992, and in 1992 a Titan 3C Transtage, SSN 3432, break-up produced at least twenty observable pieces. Subsequently several nations performed optical surveys of the GEO region in the form of independent observation campaigns. Such surveys suffer from the fact that the field of view of optical telescopes is small compared with the total area covered by the GEO ring. As a consequence only a small volume of the orbital element-magnitude-space is covered by each individual survey. Results from these surveys are thus affected by observational biases and therefore difficult to compare. This paper describes the development of a common search strategy to overcome these limitations. The strategy optimizes the sampling for objects in orbits similar to the orbits of the known GEO population but does not exclude the detection of objects with other orbital planes. A properly designed common search strategy clearly eases the comparison of results from different groups and the extrapolation from the sparse (biased) samples to the entire GEO environment.     

丁羟推进剂拉伸断裂行为的扫描电镜研究

利用扫描电镜及附属微型动态拉伸装置实验手段，对丁羟基复合固体推进剂进行了断口微观形貌观察和电镜微型拉伸试件在应变状上的断裂行为分析。结果表明，从推进剂拉伸力学行为的微观结构变化以预示其宏 同力学性能，改善丁羟推进剂粘合剂与固体颗粒之间的界面性质，是固体推进剂力学性能的一个重要方向。     

相变光盘的介质优选及理论计算

 本文着重论述相变光盘的存储机理、介质优选、理论计算及光存储最新进展。     

功率谱密度(PSD)在评价超精密光学表面中的应用研究

用原子力显微镜对不同工艺下获得的超光滑反射镜基片进行了功率谱密度(PSD)检测,并对结果进行分析,以指导光学元件加工。     

飞机变形自动化测量方法研究

为解决以往飞机变形测量模式中人工干预较多,受测量环境影响较大,测量时间长等问题,基于Geo COM技术和RS232,在计算机与全站仪之间进行数据交换,设计了一套自动化测量系统。在测量过程中由标志点的机体理论坐标反算其在当前测站中的极坐标,从而在测量过程中驱动全站仪指向待测点,减少人工瞄准时间,并由计算机实时解算结果数据。经实际飞行试验验证表明,测量时间缩短为原来时间一半,大大提高了工作效率。     

ASTROSAT

The ASTROSAT satellite is an Indian National Space Observatory under development in India. Due for launch in 2010, ASTROSAT will carry a complement of five scientific instruments enabling simultaneous observations from the optical through to the hard X-ray energy band. This capability will enable broad-band spectroscopy and high time-resolution monitoring of both galactic and extra-galactic targets, such as X-ray binaries and AGN. One of the instruments is being built in collaboration with the Canadian Space Agency and another in collaboration with the University of Leicester. ASTROSAT also carries a scanning sky monitor to observe the variable X-ray sky. After an initial period of science verification and guaranteed time, a certain fraction of ASTROSAT observing time will also be made available to the community via a call for proposals. Here I summarise the instrument complement and principle scientific objectives of the mission.