检测斜拉索张力的振动法及其应用

介绍了检测斜拉索张力的振动方法,并结合现场测试工作讨论了索力测量系统的硬件和软件设计。针对环境随机激励下斜拉索的低阶自振频率不容易识别的问题,研究了瞬态激励的检测试验方案和检测技术。工程实际应用表明:振动法检测斜拉索张力简便实用,所需仪器设备极易携带,检测结果可靠、精度高,且能满足工程应用要求。     

一种新型弹载印刷振子天线

介绍一种S波段的弹载印刷振子天线,该天线由印刷振子激励、能够摆脱弹体影响且具有朝前辐射方向 图。     

NOVEL HIGH-SPEED FPGA-BASED FFT PROCESSOR

A novel architecture for computing the fast Fourier transform ( FFT ) on programmable devices is presented.To improve the system operation speed , a hybrid parallel FFT algorithm is used.Results indicate that the use of an 8×8parallel structure for realizing the 64-point FFT leads to a 8times higher processing speed compared with its counterparts employing other series of techniques.     

基于航空货运网络结构的城市层级分析

航空货运网络是影响城市层级结构的重要因素之一,对其进行量化分析具有十分重要的理论和现实意义。根据2002—2008年中国航空货运数据库构建的中国航空货运网络,运用复杂网络分析的测度方法,以城市航空货运量比例为依据,将中国航空货运网络分成初始层级网络、中级层级网络和核心层级网络3个层次。基于航空货运网络视角,将中国通航城市分成核心、中级和边缘城市3类层级。通过对平均路径长度、聚类系数、度分布、密度等网络特征的分析,证明了3个层级城市所在的网络都具有小世界和无标度特性,研究表明中国城市层级结构具有金字塔特性,分布严重不均匀,值得关注。     

信息系统集成方面的若干问题

对信息系统集成中的信息集成,功能集成,平台集成、人的集成等几方面的问题进行了研究,在此基础上提出了一种系统集成的方法,即以信息集成为目标,功能集成为基本框架,平台集成为技术基础,人的集成为根本保证的全方位信息系统集成.文中结合某航空公司信息系统集成实例来说明这种全方位信息系统集成的方法,对信息系统集成具有一定的理论指导意义.     

异常SSC事件的行星际原因分析

磁暴急始(SSC)是强烈太阳风动压或行星际激波与磁层相互作用的结果.通常SSC事件的上升时间在4～10 min,我们把上升时间超过15 min的SSC事件称为异常SSC事件.本文利用地磁SYM-H指数鉴别出了5个有地磁观测历史以来发生的上升时间大于15 min的异常SSC事件,并利用Wind,ACE,IMP 8,Goes,Geotail多点卫星太阳风观测数据和地磁观测数据,分析了异常SSC事件的行星际原因.结果表明,异常SSC事件通常都是强烈行星际扰动引起的,5个异常SSC事件有4个对应于行星际激波,有3个对应于多步太阳风动压跃变,有1个对应于行星际电场大幅度变化;由行星际激波产生的异常SSC事件,其上升时间依赖于行星际激波的方向,方向相对于日地连线越偏,上升时间越长;异常SSC事件上升时间与行星际磁场方向关系不明显.      

多线程异地备份发动机数据软件设计与应用

通过开发发动机信息管理系统后台数据的异地备份软件,介绍了以Delphi 10 Seattle为开发工具,应用Indy组件,多线程方式实现客户端向服务器端发送备份指令,完成数据的备份、加密压缩以及向异地客户端推送数据,以客户端完成压缩数据的接收结束异地传输,同时服务器端实时向不同客户端发送执行过程信息.因发动机数据量较大,备份和传输时间较长,在异地客户端采用同步进度条显示.软件设计采用TCP可靠传输,提高数据传输的安全性.     

Formation control using μ-synthesis for Inner-Formation Gravity Measurement Satellite System

Inner-Formation Gravity Measurement Satellite System (IFGMSS) is used to map the gravity field of Earth. The IFGMSS consists of two satellites in which one is called “inner satellite” and the other one is named as “outer satellite”. To measure the pure Earth gravity, the inner satellite is located in the cavity of the outer satellite. Because of the shield effect of the cavity, the inner satellite is affected only by the gravitational force, so it can sense Earth gravity precisely. To avoid the collision between the inner satellite and the outer satellite, it is best to perform a real-time control on the outer satellite. In orbit, the mass of the outer satellite decreases with the consumption of its propellant. The orbit angular rate of the inner satellite varies with time due to various disturbing forces. These two parameters’ uncertainties make the C–W function be not so accurate to describe the formation behavior of these two satellites. Furthermore, the thrusters also have some uncertainties due to the unmodelled dynamics. To cancel the effects caused by the above uncertainties, we have studied the robust control method based on the μ-synthesis. This μ-synthesis eliminates the conservativeness and improves the control efficiency comparing with the H_∞ method. Finally, to test the control method, we simulate an IFGMSS mission in which the satellite runs in a sun synchronous circular orbit with an altitude of 300 km. The simulation results show the effectiveness of the robust control method. The performances of the closed-loop system with the μ-controller are tested by the μ-analysis. It has found that the nominal performance, the robust stability and the robust performance are all achieved. The transient simulation results further prove the control response is fast and the accuracy of the relative position meets the demand of the gravity measurement.     

航天器控制软件可靠性工程方法研究

当前航天器控制软件的复杂度越来越高,软件的规模十分庞大,对软件可靠性安全性要求极高,因此对航天器控制软件的可靠性设计和度量具有重要意义.介绍和分析适用于航天器控制软件的可靠性设计方法,并结合某型号给出实际的软件设计以及可靠性度量的具体实例.     

Effect of the Interplanetary Electric Field on the Magnetopause From Global MHD Simulations

The north-south component B_z of the Interplanetary Magnetic Field (IMF) and solar wind dynamic pressure P_d are generally treated as the two main factors in the solar wind that determine the geometry of the magnetosphere. By using the 3D global MHD simulations, we investigate the effect of the Interplanetary Electric Field (IEF) on the size and shape of magnetopause quantitatively. Our numerical experiments confirm that the geometry of the magnetopause are mainly determined by P_dB_z, as expected. However, the dawn-dusk IEFs have great impact on the magnetopause erosion because of the magnetic reconnection, thus affecting the size and shape of the magnetopause. Higher solar wind speed with the same B_z will lead to bigger dawn-dusk IEFs, which means the higher reconnection rate, and then results in more magnetic flux removal from the dayside. Consequently, the dayside magnetopause moves inward and flank magnetopause moves outward.