微小卫星平台公共总线技术——CAN网络应用

对局域控制网络(CAN)协议在“清华一号”微小卫星平台上的应用作了描述。提出了微小卫星对平台公共总线的要求,介绍了CAN网络的特点,阐述了CAN协议的帧结构,并在此基础上提出了针对卫星子系统数据通讯所作的改进协议。还给出了微小卫星星载计算机子系统的CAN节点硬件设计结构和软件控制流程。     

CPMIS综合查询及数据维护技术方法与功能分析

通过对产品管理信息系统工作情况的分析，介绍了实现综合查询及数据维护部分的技术方法，并对其功能进行了具体的剖析。     

基于使命任务分解的航空电子跨平台通信组织与仿真

在先进的综合化航空电子系统设计中,跨平台通信的组织将直接体现使命任务的需求。通过功能流程框图将航空电子系统使命任务各个阶段分解为功能组件,给出了一种功能组件之间跨平台信息交互的组织方法,并采用移动自组织通信的方式实现。将某任务片段中的空中图像信息传输作为模拟案例,使用OPNET软件进行仿真研究。仿真结果表明,该方法根据任务的特性设定平台之间的动态通信过程,与没有经过使命任务分解设计的对照组相比,在同等发射功率下能够有效地降低误码率。     

动态神经网络的稳定性分析

应用李亚普诺夫稳定性理论推导出Ｈｏｐｆｉｅｌｄ网络绝对稳定的充分条件。对本文的结果与其它Ｈｏｐｆｉｅｌｄ网络稳定性判据的关系作出讨论。为Ｈｏｐｆｉｅｌｄ网络稳定性分析提供了新的途径。     

Simultaneous observations of the plasma density on the same field line by the CPMN ground magnetometers and the Cluster satellites

By applying the cross-phase method and the amplitude-ratio method to magnetic field data obtained from two ground stations located close to each other, we can determine the frequency of the field line resonance (FLR), or the field line eigenfrequency, for the field line running through the midpoint of the two stations. From thus identified FLR frequency we can estimate the equatorial plasma mass density (ρ)$(\rho )$ by using the T05s magnetospheric field model [Tsyganenko, N.A., Sitnov, M.I. Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms, J. Geophys. Res. 110, A03208, 2005] and the equation of Singer et al. [Singer, H.J., Southwood, D.J., Walker, R.J., Kivelson, M.G. Alfven wave resonances in a realistic magnetospheric magnetic field geometry, J. Geophys. Res. 86 (A6) 4589–4596, 1981].     

直流电源输出阻抗测量技术

直流电源输出阻抗是新的特性参数,一些电源产品开始把它列入技术指标手册中。本文分析了电源阻抗的定义,总结了电源阻抗的特点,综述了当前电源阻抗测量技术的现状,提出了基于数字电桥的一种测量方法,提出了直流电源阻抗测量中的技术难点和尚待解决的技术问题。     

A mars communication constellation for human exploration and network science

This paper analyses the possibility of exploiting a small spacecrafts constellation around Mars to ensure a complete and continuous coverage of the planet, for the purpose of supporting future human and robotic operations and taking advantage of optical transmission techniques. The study foresees such a communications mission to be implemented at least after 2020 and a high data-rate requirement is imposed for the return of huge scientific data from massive robotic exploration or to allow video transmissions from a possible human outpost.     

基于信息化建设的产品合同精益管理

介绍了大型军工企业产品合同信息的创新管理，即运用创新管理理念，通过园区网，应用数据库和软件开发及网络技术实现了产品合同信息的网络数字化管理，包括合同内容、合同履行情况、付款情况等方面的过程管理，通过网络实现合同信息的快速查询、产品生产的过程监控、合同款管理的办公自动化，提升了企业产品合同管理的精益化管理。     

Correlation between the cosmic noise absorption calculated from the SARINET data and the energetic particles measured by MEPED: Simultaneous observations over SAMA region

The cosmic noise absorption is presented in terms of two-dimensional images obtained from the imaging riometers operated at the Southern Space Observatory (geographic coordinate: 29.4° S, 53.1° W), in São Martinho da Serra, Brazil, Concepcion (geographic coordinate: 36.5° S, 73.0° W) and Punta Arenas (geographic coordinate: 53.0° S, 70.5° W) in Chile, which belong to the South American Riometer Network and are located at the central and periphery regions of the South American Magnetic Anomaly. Correlations are performed between the maximum cosmic noise absorption observed at these stations and the energetic electron flux in two energy channels (>30 and >300 keV) and the proton flux in three energy channels (80–240, 800–2500 and >6900 keV) as measured by the Medium Energy Proton and Electron Detector, during a moderate geomagnetic storm that occurred on September 3, 2008. The results show high correlations between the cosmic noise absorption detected at São Martinho da Serra and the flux of protons with energy between 80 and 240 keV, and the flux of electrons with energies higher than 300 keV, while an additional ionization at Concepcion was correlated with electrons of energies higher than 30 keV. The cosmic noise absorption detected at Punta Arenas was probably caused by the increase of the protons flux with energy between 80 and 240 keV.     

航天测控资源应用现状及综合利用研究

针对我国航天测控资源存在“条块分割、设备分散”等问题,进行相应分析并提出解决设想,其目的是找到适合我国国情的航天测控资源合理配置,实现测控资源和空间资源充分共享及综合利用。首先对我国地球同步卫星和近地卫星的航天测控资源应用现状进行分析;其次根据不同卫星的测控特点,提出航天测控资源综合利用的设想,并对其利弊进行了详细讨论;最后结合我国航天测控资源实际情况,指出了实现航天测控资源综合利用需要重点解决测控覆盖范围等关键技术问题。