A hybrid,self-adjusting search algorithm for optimal space trajectory design

The aim of the present paper is to propose a hybrid, self adjusting, search algorithm for space trajectory optimization. By taking advantage of both direct and indirect methods, the present algorithm allows the finding of the optimal solution through the introduction of some new control parameters, whose number is smaller than that of the Lagrange multipliers, and whose range is bounded. Eventually, the optimal solution is determined by means of an iterative self-adjustment of the search domain occurring at “runtime”, without any correction by an external user. This new set of parameters can be found through a reduction process of the degrees of freedom, obtained through the transversality conditions before entering the search loop. Furthermore, such a process shows that Lagrange multipliers are subject to a deep symmetry mirroring the features of the state vector. The algorithm reliability and efficiency is assessed through some test cases, and by reproducing some optimal transfer trajectories: a full three-dimensional, minimum time Mars mission, an optimal transfer to Jupiter, and finally an injection into a circular Moon orbit.     

基于Internet的视频流技术研究

 Internet 服务质量( QoS) 的时空波动性给设计和实现Internet 实时视频流系统提出了巨大的挑战。以终端系统为研究对象, 给出了端到端的Internet 视频流系统结构, 建立了基于Gilber t 模型的信道包丢失率计算方法, 提出了位率自适应视频流协议SAVSP。实验结果表明, 所提出的视频流系统结构合理, SAVSP 协议性能优于目前主流的AIMD 协议。     

因特网实时动态GPS"智能桥梁"的设计与实施

介绍了基于因特网的实时动态GPS在大型结构变形监测中应用的原型系统的概念与设计.该系统包括参考基站、监测站、控制中心和用户4部分.文中采用了模拟桥梁变形的仿真平台验证该原型系统.实验结果表明:在10 Hz的采样率下,该系统的数据传输时间延迟可以忽略不计, 并可达到毫米级的三维定位精度.     

互联网逻辑重构技术发展与现状

本文主要介绍关于PLDs的互联网逻辑重构技术的概念思路，以及此技术实现的基本框架，并对一种标准的文件格式JBC的生成和通过JTAG端口配置到可编程器件进行了说明。     

利用DataSocket远程控制Fluke8840A

通过Internet或局域网将GPIB接口仪器组成分布式远程测试系统,是当前测控领域应用开发的热点问题之一,针对这一问题,本文在简述了DataSocket技术基本概念的基础上,以Fluke8840A数字电压表为例,介绍了在LabVIEW编程开发环境下,利用控件DataSocket属性、函数和VISA函数,通过局域网对GPIB接口仪器设备进行控制的方法,该方法可以充分利用GPIB接口仪器程控功能,适用于多种工业现场对象的测量、控制和现场监测,实践证明对推动GPIB接口仪器实现网络化测试,具有广泛的借鉴价值和应用价值。     

Dynamics of the convection in the inner magnetosphere by observations of the diffuse aurora,SAR arc and ionospheric drift

The first results of the comparison of subauroral luminosity dynamics in 557,7 and 630,0 nm emission with simultaneous measurements of the ionospheric drift in the F2 region with a digisonde DPS-4 at the Yakutsk meridian (CGMC: 55–60N, 200°E) at Kp = 2–6 are presented. It is shown from the analysis of individual events that during the magnetospheric convection intensification after the turn of the IMF B_z – component to the south the equatorward extension of diffuse aurora takes place. At the same time the westward ionospheric drift velocity increases both in the diffuse aurora region and much equatorward of it due to the occurrence of the northward polarization electric field. We suppose that the generation of polarization field can be associated with the development of the region 2 FAC during the intensification of magnetospheric convection. The comparison of ground-based observations with measurements of the plasma drift aboard the DMSP-F15 satellite has been carried out.     

网络环境中安全防御措施的研究

随着网络带宽增加和网络应用的日益丰富,网络受到频繁的攻击,这种攻击采用了结合病毒、蠕虫、后门等多种方式,本文详细分析了蠕虫病毒及木马、黑客对网络的侵入和威胁,提出了安全防御措施,并阐述了利用Windows2003提供的防火墙为网络构筑安全防线的方法,Internet连接防火墙可以有效地栏截对Windows2003服务器的非法入侵,防止非法远程主机对服务器的扫描,提高Windows2003服务器的安全性,如果在用Windows2003构造的虚拟路由器上启用此防火墙功能,能够对整个内部网络起到很好的保护作用.     

Mid-Latitude Pc1, 2 Pulsations Induced by Magnetospheric Compression in the Maximum and Early Recovery Phase of Geomagnetic Storms

We investigate the properties of interplanetary inhomogeneities generating long-lasting mid-latitude Pc1, 2 geomagnetic pulsations. The data from the Wind and IMP 8 spacecrafts, and from the Mondy and Borok midlatitude magnetic observatories are used in this study. The pulsations under investigation develop in the maximum and early recovery phase of magnetic storms. The pulsations have amplitudes from a few tens to several hundred pT andlast more than seven hours. A close association of the increase (decrease) in solar wind dynamic pressure (Psw) with the onset or enhancement (attenuation or decay) of these pulsations has been established. Contrary to high-latitude phenomena, there is a distinctive feature of the interplanetary inhomogeneities that are responsible for generation of long-lasting mid-latitude Pc1, 2. It is essential that the effect of the quasi-stationary negative Bz-component of the interplanetary magnetic field on the magnetosphere extends over 4 hours. Only then are the Psw pulses able to excite the above-mentioned type of mid-latitude geomagnetic pulsations. Model calculations show that in the cases under study the plasmapause can form in the vicinity of the magnetic observatory. This implies that the existence of an intense ring current resulting from the enhanced magnetospheric convection is necessary for the Pc1, 2 excitation. Further, the existence of the plasmapause above the observation point (as a waveguide) is necessary for long-lasting Pc1 waves to arrive at the ground.      

强磁场结构在行星际空间膨胀的数值模拟

本文研究了强磁场结构在18—240R_s的行星际空间的膨胀效应。模拟结果表明, 强磁场结构的膨胀能够形成典型的磁云剖面结构;膨胀速度明显依赖于磁场强度的大小;强磁场结构运动的速度直接影响到它的动力学特性。