深空探测中利用静止轨道卫星编队连续导航精度分析

针对我国难以全天候24小时对探测器连续测控和通信，以及建立全球性深空网络困难的问题，提出利用地球静止轨道卫星编队进行深空导航的构想。两个静止轨道卫星编队相距一定角度，可以完成对深空探测器进行全天候连续导航定位。卫星编队采用无源反向导航的方法，多颗卫星协同工作，共同完成导航任务。分析表明该天基导航系统的几何参数精度因子受时间测量误差均方差和基线长度变化影响较大。编队的构型对定位精度有很大影响，其中基线长度不能过小，时间测量误差均方差不能过大，否则定位误差会急剧增加，伴随卫星椭圆轨道偏心率也存在一定界限。增加伴随卫星数量也有利于提高系统的定位精度。     

深空通信中的Turbo码技术

简介深空通信的发展现状和 Turbo码的基本原理。着重研究深空通信中 Turbo码技术的算法和应用 ;并通过仿真对 Turbo码和其它传统码的性能进行比较分析。针对深空通信的特点 ,就 Turbo码具体实现的技术作了探讨     

人工智能在OODA 循环中的应用

当前人工智能(AI) 是商业和工业，甚至军事应用领域中最热门的流行语。军事国防领域也已经将人 工智能发展成为了一种技术，并应用到军事作战和决策系统中。最初OODA 循环是最知名的空战战术模型， 后来发展成为各国空军的作战方法。OODA 循环对于任务的定义和决策过程的理解起到了重要的作用。本文主 要研究了人工智能在OODA 循环决策中的应用。讨论了未来OODA 循环各阶段中所需的AI 作用和技术，包 括可解释的人工智能和基于学习的人工智能。     

CFDP协议中延迟NAK文件传输时间分析与仿真

未来的深空通信需要一个鲁棒的、有效与可靠的文件传输协议,在研究CCSDS提出的CFDP协议基础上,针对延迟NAK模式提出了一种新的分析方法。在保证吞吐量的前提下,对ARQ定时器优化设置,导出了平均文件传输时间的理论表达式。在单跳直连链路中,对不同条件下的平均文件传输时间进行了仿真与数值分析。仿真结果表明平均文件传输时间与PDU错误概率、PDU数目及单向传播时间等有密切关系。随机仿真与理论分析具有很好的一致性。     

电子技术基础课程研究型教学模式的探索与实践

本文首先阐明对培养学生创新意识培养的认识,然后讲述怎样结合电子技术基础课程的特点建立研究型教学模式,进而介绍丰富的教学实践,以及多层次、系列化和立体化的教材建设,最后说明教学效果。     

Fronts and thermohaline structure of the Brazil–Malvinas Confluence System

Fronts and thermohaline structure of the Brazil–Malvinas Confluence System (BMCS) are studied from climatic data, “Marathon Exp. Leg.8, 1984” data, and Sea surface temperature (SST) data base “ds277-Reynolds” (1981–2000). The South Atlantic Central Water (SACW) is divided in two main types: tropical (TW) and subtropical water (ST). Water masses, Fronts, Inter-Frontal and Frontal Zones are analysed and classified: (a) the water masses: Tropical Low-Salinity Water, Tropical Surface Water, Tropical Tropospheric Water, Subtropical Low-Salinity Water, Subtropical Surface Water, Subtropical Tropospheric Water. T,S characteristics of intermediate, deep and bottom water defined by different authors are confirmed and completed; (b) the Inter-Frontal Zones: Tropical/Brazil Current Zone, Subtropical Zone and Subantarctic Zone; (c) the Frontal Zones: Subtropical, Subantarctic and Polar, and (d) the Fronts: Subtropical Front of the Brazil Current, Principal Subtropical Front, North Subtropical Front, Subtropical Surface Front, South Subtropical Front, Subantarctic Surface Front, Subantarctic Front and Polar Front. Several stable T–S relationships are found below the friction layer and at the Fronts. The maximum gradient of the oceanographic characteristics occurs at the Brazil Current Front, which can be any of the subtropical Fronts, depending on season. Minimum mean depth of the pycnocline coincides with the Fronts of the BMCS, indicating the paths of low-salinity shelf waters into the open ocean. In the work it is shown how to recover the horizontal and vertical thermohaline structure of waters from satellite data RSMAS SST.     

基础振动影响下微g加速度计静态数学模型辨识

以从俄罗斯引进的低频微g加速度计校准装置为基础,分析了基础振动对微g加速度计校准结果的影响,给出了消除基础振动噪声的方法及在该种情况下加速度计静态数学模型的辨识方法.     

NASA深空网（DSN）的现状及发展趋势

详细介绍了美国深空网的发展过程、目前的状况以及未来的主要发展计划。     

机场道面动态响应分析

 本文首先研究了粘弹性地基上四边自由矩形板在运动载荷作用下的动态响应问题,得到了问题的近似解答。然后从该解答出发讨论了机场道面的动态响应问题,并以××机场道面板为计算模型,将理论计算结果和实验结果进行比较,二者符合较好。最后计算了道面的固有频率、临界速度,讨论了主要物理参数对道面动挠度的影响规律。     

The Coma of Comet 9P/Tempel 1

As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 10² km), it is in collisional equilibrium, at larger distances (≥10⁴ km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics of the coma, as well as with its variability with time, orbital position, and heliocentric distance. The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986. This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards that the coma presents for the spacecraft. An erratum to this article is available at .