分布式处理在民航生产中的应用

阐述了分布式计算机系统的基本原理以及互连方式,对其功能、特点进行了分析.为使该系统在民航等系统中的应用和研究更加广泛,文中还给出了一些应用实例.     

Local clouds: Distribution, density and kinematics through ground-based and HST spectroscopy

The distribution, kinematics and physical properties of the interstellar matter surrounding the Sun can be inferred from ground-based and UV spectroscopic observations. On a 200 pc scale the local interstellar matter appears inhomogeneous and asymmetric. Although it generally flows towards the lower density region, it is composed of numerous small components a few parsecs in size with slightly different velocities. On a smaller scale the extent and the nature of the Local Cloud which flows over the Sun are discussed based on HST-GHRS observations of nearby stars.     

浅谈如何发挥高校实验室的作用

本文主要阐述了实验的重要性和实验教学的重要地位，实验教学观念转变及实验室如何建设发展，实验室的建设发展对高等院校教学与科研的重要作用，对高等院校的知名度和经济效益，吸引人才等方面起到的推动作用。     

基于排队论的防空部署效率分析

为简化空防对抗中防空部署效率的分析,提出了一种基于排队论的分析方法。将作战过程视为先到先服务的服务系统,在目标持续入侵时目标流作为泊松申请,近、中/远程地空导弹武器集群分别为带失效和有限等待时间的排队系统。在一定的简化条件下建立了两种火力单元部署效率的数学模型。算例表明,该法可描述我方火力单元数、武器系统毁伤能力(服务时间)和空中目标流密度间的关系,能用于评估混编防空武器系统的部署效率,算法简单。     

航天器被动检漏方法的探讨

分析了航天器被动检漏的具体要求，对常用几种主要被动检漏方法进行了评述，指出了各种被动检漏方法的优、缺点和技术状态。最后，针对我国航天器的被动检漏需求，推荐了航天器被动检漏的相关措施。     

基于扩展卡尔曼滤波的GPS多径抑制技术

本文研究GPS系统中多径误差抑制技术。利用小范围多天线系统中多径对各天线之间伪距测量值影响的相关性，采用扩展卡尔曼滤波技术得到多径信号各参数，从接收信号中消去多径信号，以抑制多径信号影响。文章推导了多径信号对码环误差影响的闭合表达式，建立了采用当前统计模型的状态方程和观测方程。仿真表明该方法具备良好的抑制效果。     

RLV再入轨迹机载快速优化

为了可重复使用飞行器再入轨迹机载快速优化的需求,开发一种再入轨迹快速优化算法。根据RLV再入三维轨迹的特点,引入了新的假设,对RLV再入轨迹状态方程进行简化处理,使优化迭代计算量大大减少,在此基础上,使用乘子法对再入终端约束进行处理,然后用共轭梯度法求解优化再入轨迹,最后以美国航天飞机为例计算再入最优轨迹。结果验证该算法在满足约束条件的情况下,具有很快的收敛速度,在不同初始再入条件和终端约束条件下,计算机时一般小于一分钟。该算法具有很好的工程应用前景。     

论“三个代表”思想的时代特点

江泽民同志提出的“三个代表”的重要思想,是站在世纪之交的时代高度,总揽全局,对我党近80年历史经验和50年执政经验的总结,提出了加强执政党自身建设的新思路,创造性地发展了马克思主义党建理论与学说,具有鲜明的时代特点。本文就“三个代表”思想所体现的时代特点进行了初步的探讨,论证了其内在逻辑上的统一性,指出了“三个代表”思想必将成为新世纪党建理论的强大思想武器和伟大旗帜。     

开环全保偏光纤陀螺研究

开环全保偏光纤陀螺结构简单，有使用价值；进入９０年代国外研究成功熔接型保偏光纤耦合器以后，这种陀螺更受重视，向实用方向发展，对研究全保偏光纤陀螺中的几个关键问题，光路中元器件的特性；保偏光纤的对轴熔接技术，零漂和噪声做了分析，实验结果表明，零漂达到１．２４°／ｈ。     

Quasi-biennial oscillations in the cross-correlation of properties of macrospicules

Jets, whatever small (e.g. spicules) or large (e.g. macrospicules) their size, may play a key role in momentum and energy transport from photosphere to chromosphere and at least to the low corona. Here, we investigate the properties of abundant, large-scale dynamic jets observable in the solar atmosphere: the macrospicules (MS). These jets are observationally more distinct phenomena than their little, and perhaps more ubiquitous, cousins, the spicules. Investigation of long-term variation of the properties of macrospicules may help to a better understanding of their underlying physics of generation and role in coronal heating. Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory, a new dataset, with several hundreds of macrospicules, was constructed encompassing a period of observations over six years. Here, we analyse the measured properties and relations between these properties of macrospicules as function of time during the observed time interval. We found that cross-correlations of several of these macrospicule properties display a strong oscillatory pattern. Next, wavelet analysis is used to provide more detailed information about the temporal behaviour of the various properties of MS. For coronal hole macrospicules, a significant peak is found at around 2-year period. This peak also exists partially or is shifted to longer period, in the case of quiet Sun macrospicules. These observed findings may be rooted in the underlying mechanism generating the solar magnetic field, i.e. the global solar dynamo.