空间载荷机柜热控设计的仿真研究

空间站主动热控系统的作用是提供和保持航天员、仪器设备和结构部件所要求的温度、湿度和风速等热环境。本文以空间载荷机柜为热控系统的基本单元，建立了以单相流体循环回路为基础、采用液冷结合风冷的冷却方式的载荷机柜数学模型；介绍了模糊增量控制算法的工作原理；提出了采用模糊增量控制算法，以液冷支路进出口温差和风冷支路冷却量占总冷却量的比值为控制目标的反馈控制策略。同时文章采用数值模拟方法研究了控制系统的动态响应效果。仿真结果显示，模糊增量控制算法具有响应迅速、超调量小、无静态误差的特点，控制策略满足有效性、稳定性和高精确度的要求。     

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.     

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。     

Scientific Planning and Commanding of the Rosetta Payload

ESA’s Rosetta mission was launched in March 2004 and is on its way to comet 67P/Churyumov-Gerasimenko, where it is scheduled to arrive in summer 2014. It comprises a payload of 12 scientific instruments and a Lander. All instruments are provided by Principal Investigators, which are responsible for their operations. As for most ESA science missions, the ground segment of the mission consists of a Mission Operations Centre (MOC) and a Science Operations Centre (SOC). While the MOC is responsible for all spacecraft-related aspects and the final uplink of all command timelines to the spacecraft, the scientific operations of the instruments and the collection of the data and ingestion into the Planetary Science Archive are coordinated by the SOC. This paper focuses on the tasks of the SOC and in particular on the methodology and constraints to convert the scientific goals of the Rosetta mission to operational timelines.     

基于椭圆路径的回转二次曲面点接触加工方法研究

本文给出并证明了基于点接触的回转二次曲面加工成形原理,此加工方法加工范围广,刀具和加工面形之间具有多对多的对应特性。提出基于此成形原理的加工机床构建方案,分析加工中刀具配置要求,给出了满足配置要求的刀具配置方案。最后,设计了基于点接触成形原理的加工部件。     

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。     

光机热集成分析中数据转换接口的研究

光机热集成分析中的数据转换接口是实现光、机、热各分析软件间数据有效传递的重要手段。Zernike多项式的优点决定了它作为各分析软件间的数据接口工具是非常方便和成熟的。以一种数据处理算法和最小二乘法为Zernike多项式拟合的基础,编制了数据转换接口,实现了分析模块间数据的转换,并在某空间遥感器主镜系统的光机热集成分析中得到应用。     

卫星微波遥感定标技术

在简要论述微波遥感定标技术工作特点的基础上，着重分析星载有源微波遥感定标技术基本原理和关键技术，比较了各种定标方法特点，提出了若干建议。     

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。     

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.