基于有向图模型的卫星任务指令生成算法

面向任务的卫星操控模式具有操作简便、星载资源使用效率高的优点,正在取代指令序列注入成为遥感卫星运控的新模式。文章提出一种基于有向图模型的遥感卫星任务指令序列生成算法,具有线性存储复杂度和计算复杂度,适合存储资源和计算资源受限的星载计算机应用。此算法已在某遥感卫星应用,测试试验表明,采用3个面向任务的高级指令即可生成52种指令序列,任务上行注入效率提升了5倍。本文方法根据有效载荷的使用约束条件,配置有向图模型参数,即可满足各种类型卫星使用。     

电极面型对横向激励高气压CO2激光器放电的影响

计算并讨论了均匀场电极中电极板安装结构、电极板厚度对实际电场分布影响。计算表明在基本参数类似的条件下,近罗可夫斯基电极表面电场强度具有17%的非均匀性,但在垂直放电方向的对称面上却有更好的均匀性。对放电区辉光的时间积分照片和像增强型CCD相机记录的瞬态照片进行了分析,结果表明:电极表面的电场强度分布,仅对放电的初始发展具有影响,而放电区中央的电场分布以及预电离强度,对最终放电区的均匀性具有决定性的影响。     

航迹规划中雷达探测空间的生成

从飞机突防习行任务规划出发，综合考虑地球曲率、陆地（或海洋）的反射和杂波干扰、大气折射和吸收损耗等因素的影响，采用临界散射截面法生成了对空警戒雷达在不同地貌、发现概率下，对不同雷达散射截面的目标的探测空间。计算并分析了飞行高度、目标雷达散射截面、发现概率和地貌等因素对雷达探测空间的影响，以便选择低探测概率的飞行走廓，这对制定和实施安全突防飞行策略有实际意义。     

Deep Impact Mission Design

The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment. The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth.     

Propagation of interplanetary shocks into the Earth’s magnetosphere

This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper.     

Current status of the BepiColombo/MMO spacecraft design

This paper shows the current baseline of the conceptual design of the BepiColombo/MMO (mercury magnetospheric orbiter) spacecraft, which is conducted by the ISAS Mercury Exploration Working Group. The MMO is a spinning spacecraft of 200 kg mass whose spin axis is nearly perpendicular to the Mercury orbital plane. The current status of the overall MMO system and subsystems such as thermal control, communication, power, etc. are described. The latest status of the development of critical technologies for the MMO and the outline of the international cooperation between ESA and ISAS are also presented.     

UML在软件可靠性测试数据自动生成中的运用

为了自动生成实时嵌入式软件的可靠性测试数据,利用UML(统一建模语言)提供的建模机 制,从软件可靠性测试的角度建立use-case剖面、接口模型和测试数据实现模型,然后根 据 这些模型的描述进行随机抽样,自动生成可靠性测试数据.利用该方法能够开发出相应的测 试数据自动生成工具,在软件可靠性测试领域有着较大的实用价值.     

X射线天文卫星观测需求分析与控制总体设计

对X射线天文卫星观测需求进行了分析,提炼了观测任务对观测模式、源的高精度定位与对准、轨道、热控、测控数传等多项需求与约束;针对X射线观测的多需求、多约束难点,设计了集巡天观测、定点观测与小天区扫描观测于一体的观测模式,解决了一颗卫星同时实现全天扫描、银道面深度扫描、重要惯性区域扫描、重要及机遇目标深度观测以及伽马暴全天监测的多种观测需求的难题,该技术已在我国硬X射线调制望远镜卫星上得到应用.     

改进的遥感卫星成像任务单轨最优团划分聚类方法

针对遥感卫星成像任务规划时对点目标的聚类效果不佳的问题,提出了一种改进的单轨最优团划分聚类方法。根据聚类约束条件,构建任务聚类图模型,并为图模型中的每一条边赋权值;根据图模型中边的权值,构建权值矩阵P;以卫星单轨姿态机动的最大次数作为聚类任务的数量限制,由P依次计算每个聚类任务所有可能的最优聚类方案,并生成对应的收益矩阵M和终点矩阵N;通过循环遍历的方式计算各个聚类方案下的总收益,其中总收益最大的方案即为最优团划分聚类方案。仿真结果表明:提出的改进的团划分聚类方法,能将点目标有效聚类,与传统任务聚类方法相比,可明显提高遥感卫星对点目标的观测效率。研究结果可为我国遥感卫星自主任务规划技术研究提供参考。     

基于任务段的航空发动机载荷谱聚类方法

针对航空发动机飞行任务剖面分类问题,对发动机31个飞行任务剖面进行了聚类分析。选取飞行高度和飞行马赫数作为划分飞行任务剖面的参数, 依据其对应的飞行任务段均值生成聚类散点图,将剖面类型划分为5大类。结果表明:低空低速剖面在无量纲飞行高度为0~0.2、飞行马赫数为0.4~0.6区间,均值最低;高空高速剖面在无量纲飞行高度为1.2~2.2、飞行马赫数为1.0~1.8区间,均值最高;飞行任务剖面在无量纲飞行高度为0.2~1.2、飞行马赫数为0.6~1.0区间内最为集中;针对散点密集区域,可依据剖面特征进一步划分剖面类型;不同剖面间,飞行高度与飞行马赫数差异性强,利于剖面划分,而法向过载与转速差异性小,不利于剖面的划分。所提出的方法可以快速有效的对航空发动机飞行任务剖面进行聚类分析。