Generic procedure for designing and implementing plan management systems for space science missions operations

This paper is one of the components of a larger framework of activities whose purpose is to improve the performance and productivity of space mission systems, i.e. to increase both what can be achieved and the cost effectiveness of this achievement. Some of these activities introduced the concept of Functional Architecture Module (FAM); FAMs are basic blocks used to build the functional architecture of Plan Management Systems (PMS). They also highlighted the need to involve Science Operations Planning Expertise (SOPE) during the Mission Design Phase (MDP) in order to design and implement efficiently operation planning systems. We define SOPE as the expertise held by people who have both theoretical and practical experience in operations planning, in general, and in space science operations planning in particular. Using ESA’s methodology for studying and selecting science missions we also define the MDP as the combination of the Mission Assessment and Mission Definition Phases. However, there is no generic procedure on how to use FAMs efficiently and systematically, for each new mission, in order to analyse the cost and feasibility of new missions as well as to optimise the functional design of new PMS; the purpose of such a procedure is to build more rapidly and cheaply such PMS as well as to make the latter more reliable and cheaper to run. This is why the purpose of this paper is to provide an embryo of such a generic procedure and to show that the latter needs to be applied by people with SOPE during the MDP. The procedure described here proposes some initial guidelines to identify both the various possible high level functional scenarii, for a given set of possible requirements, and the information that needs to be associated with each scenario. It also introduces the concept of catalogue of generic functional scenarii of PMS for space science missions. The information associated with each catalogued scenarii will have been identified by the above procedure and will be relevant only for some specific mission requirements. In other words, each mission that shares the same type of requirements that lead to a list of specific catalogued scenarii can use this latter list of scenarii (regardless of whether the mission is a plasma, planetary, astronomy, etc. mission). The main advantages of such a catalogue are that it speeds-up the execution of the procedure and makes the latter more reliable. Ultimately, the information associated to each relevant scenario (from the catalogue or freshly generated by the procedure) will then be used by mission designers to make informed decisions, including the modification of the mission requirements, for any missions. In addition, to illustrate the use of such a procedure, the latter is applied to a case study, i.e. the Cross-Scale mission. One of the outcomes of this study is an initial set of generic functional scenarii. Finally, although border line with the above purpose of this paper, we also discuss multi-spacecraft specific issues and issues related to the on-board execution of the plan update system (PUS). In particular, we show that the operation planning cost of N spacecraft is not equal to N times the cost of 1 spacecraft and that on-board non-synchronised operation will not require inter-spacecraft communication. We also believe that on-board PUS should be made possible for all missions as a standard.     

一种采用线性光耦实现温度隔离测量的方法CSCD

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基于Casper和Simulink的射电谱仪信号处理系统设计与实现

基于Casper硬件平台的射电望远镜数字系统正在被广泛应用.在Simulink中通过调用Casper模块可以实现复杂的数字信号设计,加快FPGA开发射电望远镜系统的效率.利用Casper模块和Simulink中Xilinx模块设计射电望远镜单元样机的数字信号处理单元,完成子带的抽取、下变频和整体频谱分析等功能.在Casper通用硬件平台ZYNQ7020上进行相关功能的仿真,验证了利用Casper模块和Xilinx模块设计基于FPGA的射电望远镜单元样机信号处理系统的可行性和高效性.      

光学镜头偏振度测试技术研究

根据斯托克斯参量计算偏振度的方法,设计了光学镜头偏振度测量仪。光学镜头偏振度测量仪采用模块化结构设计,共分为光源系统、准直光学系统、载物转台、探测系统以及后续的信号处理和计算控制系统等五部分。测量透过被测量光学镜头的光分别在0,45,90,135振动方向光信号大小τH,τ45,τV,τ135,以及左旋圆偏振光、右旋圆偏振光信号的大小礼,Jr尺,计算出光学镜头的偏振度;通过对测量装置的分析,找出了影响测试结果的几个因素,并由此分析了不确定度的来源,建立了测量不确定度的数学模型,得到了装置的扩展不确定度约为0．5％。     

飞机微波着陆模拟器自动计量系统研制CSCD

本文首先简述了MLS模拟器及其计量性能要求,然后对研制的MLS模拟器自动计量系统进行了详细介绍,包括硬件分系统组成及其关键技术,软件分系统架构及其核心流程;最后将自动计量系统应用于多台MLS模拟器的校准/检定。应用表明,MLS模拟器自动计量系统能够解决MLS模拟器计量保障中存在的问题,确保MLS机载设备各项参数准确一致,进而保证了飞行安全。     

关于角度量列为基本量的探讨

在SI国际单位制中,平面角是导出量,平面角的单位“弧度”是辅助单位。但是,平面角既不能由长度基本单位导出,又不能溯源至长度基本单位,因此不能确立导出关系。平面角应用广泛,作用重要,具有独特的性能,符合基本量的要求,因此提出：平面角,简称“角度”,是基本量;平面角的单位“度、（角）分、（角）秒”,是基本单位,以供探讨。     

驱动卫星捕获碎片的电子回旋共振离子推力器系统优化

近年来空间碎片数量急剧增加,已经对空间飞行器造成了严重的威胁。为此提出在碎片密集区域轨道(700km～1000km高度)的碎片处理方案,即利用微小卫星在电子回旋共振(ECR)离子微推进连续切向力作用下,不断进行轨道提升并进行碎片收集。基于此,进一步对电推进系统方案进行优化设计计算,在设计寿命1年的条件下,以推进系统质量最低作为优化目标,以加速电压和工质流量为变量,对电推进系统方案进行优化。最终得到的优化结果为工质流量0.25sccm (0.0244mg/s)、加速电压2488V时,推进系统总体最优,总质量7.288kg,推力器比冲2216s,推力535μN。     

氧化聚丙烯腈纤维径向异质光学显微分析

为检测整束氧化聚丙烯腈纤维径向异质结构发育情况,迫切需要开发一种评价聚丙烯腈纤维是否均质氧化的检测方法。本文通过树脂包埋和研磨抛光制备用于光学分析的纤维试样,应用光学显微方法对比分析了两种类型氧化聚丙烯腈纤维径向异质结构演变过程,提出了氧化聚丙烯腈纤维径向异质结构演变模型。结果表明,TG300氧化聚丙烯腈纤维呈典型的径向异质结构,TG800氧化聚丙烯腈纤维径向异质结构不明显。随着氧化反应进行,纤维直径和碳含量逐渐降低,而氧含量逐渐上升。这说明光学显微分析可以用于氧化聚丙烯腈纤维是否均质氧化评价,可为得到均质氧化聚丙烯腈纤维提供分析检测手段。     

基于蒙皮内形定位的飞机壁板柔性装配系统

针对飞机壁板数字化、柔性化制造需求,提出一种基于蒙皮内形定位的飞机壁板柔性装配方法,通过有限元参数化建模,应用蒙皮支撑点寻优算法,实现卡板布局优化设计.根据壁板组件各零件的定位要求,详细设计了壁板柔性装配系统中长桁、蒙皮、角片的柔性定位方式,开发了基于EtherCAT总线的分布式网络控制系统用于完成整个壁板的装配.本系...