空间机器人在轨更换ORU的力/位混合控制方法

针对ORU在轨更换任务,首先推导了空间机械臂末端自由、末端与环境接触等情况下的动力学方程,并提出了相应的接触力计算方法;其次,改进了传统的R\|C控制方法,采用加权选择矩阵代替原有的选择矩阵,实现了力控制与位置控制之间的平滑切换;最后,开发了基于Matlab/Simulink的闭环控制仿真系统,该系统由多体动力学、接触动力学、轨迹规划、力/位混合控制、3D显示等模块组成。利用该系统开展了ORU转移与安装过程的闭环控制仿真,仿真结果校验了所提方法的有效性。     

基于Patran/Nastran 和Hypersizer的复合材料后机身加筋结构形式选择分析

针对复合材料后机身加筋壁板构型选择问题,采用有限元前后置处理软件Patran建立有限元模型,使用有限元分析软件Nastran进行初步分析,利用复合材料结构分析与优化软件Hypersizer进行结构形式的优化计算分析,优选出后机身壁板最佳结构形式。通过计算分析,得出有意义的工程经验。     

Height of shock formation in the solar corona inferred from observations of type II radio bursts and coronal mass ejections

Employing coronagraphic and EUV observations close to the solar surface made by the Solar Terrestrial Relations Observatory (STEREO) mission, we determined the heliocentric distance of coronal mass ejections (CMEs) at the starting time of associated metric type II bursts. We used the wave diameter and leading edge methods and measured the CME heights for a set of 32 metric type II bursts from solar cycle 24. We minimized the projection effects by making the measurements from a view that is roughly orthogonal to the direction of the ejection. We also chose image frames close to the onset times of the type II bursts, so no extrapolation was necessary. We found that the CMEs were located in the heliocentric distance range from 1.20 to 1.93 solar radii (Rs), with mean and median values of 1.43 and 1.38 Rs, respectively. We conclusively find that the shock formation can occur at heights substantially below 1.5 Rs. In a few cases, the CME height at type II onset was close to 2 Rs. In these cases, the starting frequency of the type II bursts was very low, in the range 25–40 MHz, which confirms that the shock can also form at larger heights. The starting frequencies of metric type II bursts have a weak correlation with the measured CME/shock heights and are consistent with the rapid decline of density with height in the inner corona.     

旋转弹导引头红外角跟踪回路研究

分析了导引头红外末制导角跟踪回路的稳态性能对旋转弹跟踪性能的影响,以及起伏噪声对制导精度的影响,提出了采用二阶无静差角跟踪回路的改进办法.针对改进后的角跟踪回路,计算出了失调角和目标视线角之间的关系,并采用卡尔曼滤波将目标视线角速度准确地估计出来.试验结果表明:二阶无静差系统可以提高旋转弹的跟踪性能,且能够输出满意的制导信号,具有很好的实用价值.     

关于DBS小口径接收天线选型几个问题的探讨

一个典型的双反射面天线效率大约与１６个因子有关。本文从理论上分析了正馈和偏馈对天线效率影响的各种因素。天线偏馈能改善遮挡因子ηｂ，但同时会引发漏射效率因子、照射效率因子、交叉极化效率因子等下降、波束偏移等一系列问题。文章指出，用正馈天线具备多种优点。对于在给定Ｃ／Ｎ和ＥＩＲＰ情况下如何选择天线口径作了论述，并讨论了小口径天线Ｋｕ／Ｃ兼容、ＥＩＲＰ与天线余量等问题。     

基于信息管理与融合技术在目标类型识别上的研究

在系统模型的基础上结合实战提出影响目标飞机类型识别的证据,并按照影响程度进行优先权排序;结合数据库,提出证据概率计算的数学表达式;采用深度优先搜索的融合模式,按照D-S证据理论进行融合计算;在传感器管理模块的作用下,对融合结果进行反馈控制;结合实例,对系统进行仿真验证,证明其可靠有效。     

Relationships between energetic storm particle events and interplanetary shocks driven by full and partial halo coronal mass ejections

We have analysed energetic storm particle (ESP) events in 116 interplanetary (IP) shocks driven by front-side full and partial halo coronal mass ejections (CMEs) with speeds $>$400 km s^?1during the years 1996–2015. We investigated the occurrence and relationships of ESP events with several parameters describing the IP shocks, and the associated CMEs, type II radio bursts, and solar energetic particle (SEP) events. Most of the shocks (57 %) were associated with an ESP event at proton energies $>$1 MeV.The shock transit speeds from the Sun to 1 AU of the shocks associated with an ESP event were significantly greater than those of the shocks without an ESP event, and best distinguished these two groups of shocks from each other. The occurrence and maximum intensity of the ESP events also had the strongest dependence on the shock transit speed compared to the other parameters investigated. The correlation coefficient between ESP peak intensities and shock transit speeds was highest (0.73 $\pm$ 0.04) at 6.2 MeV. Weaker dependences were found on the shock speed at 1 AU, Alfvénic and magnetosonic Mach numbers, shock compression ratio, and CME speed. On average all these parameters were significantly different for shocks capable to accelerate ESPs compared to shocks not associated with ESPs, while the differences in the shock normal angle and in the width and longitude of the CMEs were insignificant.The CME-driven shocks producing energetic decametric–hectometric (DH) type II radio bursts and high-intensity SEP events proved to produce also more frequently ESP events with larger particle flux enhancements than other shocks. Together with the shock transit speed, the characteristics of solar DH type II radio bursts and SEP events play an important role in the occurrence and maximum intensity of ESP events at 1 AU.     

航天电连接器及其组件失效分析

介绍了航天电连接器及其组件失效分析中初步分析、详细分析、故障假设和最终鉴定四个阶段的内容及方法。阐述了断路、接触不良、瞬断、绝缘不良、短路、误配线、固定不良和密封不良等常见失效模式和失效机理。给出了失效分析的程序和若干检验方法。     

基于工艺设计过程的工作流模型

通过对工艺设计过程工作流模型的研究,将现阶段工艺规程设计的工作模式转化为计算机可处理的工作模式.介绍了建立装配大纲(AO)、制造大纲(FO)、电子审签系统的流程控制方法和运行状态,以及所开发基于工作流平台的工艺编制功能.     

基于动态故障树的故障隔离程序分析方法

传统的故障隔离程序采用常规静态故障树进行故障分析，可能会导致故障原因分析不全、故障隔离路径过于繁琐等问题。提出基于系统原理和动态故障树进行故障隔离程序分析的方法，以某飞机防火系统引气导管过热探测系统故障为实例，进行系统设计原理和故障告警逻辑分析，引入动态逻辑门，构建具有顺序相关、功能相关和备份关系的动态故障树；在此基础上进行关联故障分析和排故流程图转化。结果表明：该方法能系统地、全面地反映故障触发逻辑，提供快速、准确、有效的故障隔离程序，提高飞机维修保障水平，在复杂飞机系统的航线维修领域具有良好的应用前景和推广价值。