一种前飞状态直升机可达区域快速计算方法

直升机可达区域可用于生成空域安全态势,提高直升机在低空复杂环境中的飞行安全水平.为了满足求解可达区域的实时性和准确性要求,提出了一种快速计算方法.根据能量机动性求解了直升机控制域,结合运动学方程建立了可达区域数学模型.基于最优控制原理,实现了边界点快速计算;提出了基本可达区域的概念,将实时可达区域构造问题转化为少量边界点的计算问题.以AH-1G直升机为对象进行了二维和三维的算例分析,并与微分包含法计算结果进行了对比.算例结果表明,直升机控制域是时变的,需根据实时飞行状态进行计算;该算法能实时计算前飞状态直升机的可达区域,有较高的计算精度.     

基于最优化问题的混合再入制导方法

在深入研究机动再入飞行器标准轨道和预测制导方法的基础上,针对标准轨道和预测制导相结合的制导方法,分析了由预测制导指令延迟引起的误差,提出了误差补偿策略.根据最优化理论,设计了相关性能指标函数,提出新的预测制导算法.并结合标准轨道法,通过对有限几个特征点位置上引入预测制导,形成了一种基于最优化问题的混合制导方法.有效减小了预测制导指令的解算时间,进一步降低了落点误差.仿真结果表明,该方法既具有较强的抗干扰能力和较高的制导精度,又具有一定的工程实用价值.     

基于模糊逻辑的预测再入制导方法

在研究再入飞行器预测制导基础上,针对实时性要求,提出了一种基于模糊逻辑系统的模糊预测制导方法.首先研究分析了再入飞行器落点纵程与飞行高度、弹道倾角三者之间的联系;设计了以再入飞行器落点偏差和飞行高度为输入,弹道倾角角速度为输出的模糊逻辑系统;并在此基础上根据专家经验制定模糊规则,设计模糊预测制导算法.该方法避免了一般预测制导在形成弹道倾角修正指令时所需要的大量迭代运算,有效减小了预测制导指令的解算时间,为再入飞行器在再入过程中全程使用预测制导提供了可能.仿真结果表明:该方法实时性好,落点精度高,抗干扰能力强,且具有一定的工程实用价值.      

单片微机在控制模型姿态角中的应用

用廉价单片微机８０９８装置（包括单片机外围芯片、辅助电路、角度显示器、控制程序等），控制多台大功率步进电机，实现模型姿态角的控制，并对如何利用软件来提高步进电机的运行频率，模型姿态角β、α和下转盘进行跟踪显示等有关技术进行了探讨。     

CONTROL STRUCTURE AND IMPLEMENTATION OF CELL CONTROL SYSTEM

在计算机集成制造系统（ＣＩＭＳ）的递阶控制结构中，单元控制系统起着重要作用。它上端联接车间控制系统和ＣＡＤ／ＣＡＰＰ／ＣＡＭ系统，下端联接生产设备，直接影响到生产的柔性和效率。该系统根据生产任务和目标，完成了生产计划调度、资源分配、监控设备运行等功能。文中主要讨论了系统的控制结构、系统功能和以下主要关键技术：客户／服务体系结构在生产控制和管理中的应用，单元生产计划和调度，ＤＮＣ接口以及生产中的随机事件处理。该系统已在应用中取得良好的经济效益。     

空间通信与BATS码：天成之合

创新通信技术在国家重大空间技术开发计划中有着巨大的需求。本文综述了基于网络编码的空间通信技术,旨在探索未来基于网络编码的空间通信技术的可行性和潜力。首先讨论了空间通信的特点,并给出了不同编码方法的概述;详细介绍了基于网络编码的批量稀疏编码（BATS码）创新技术。BATS码作为一种潜在的应用技术可以很好地解决多跳中继网络中严重丢包问题;给出一个BATS码原型设计和实现,实验结果证明BATS码比现有技术具有明显优势;最后,讨论了BATS码在空间通信中的应用前景。     

零售服务质量中的人力资源管理(英文)

本文研究了人力资源管理与服务质量的关系。透过问卷调查及数据分析,确立人力资源的重点、结构与相互关系,促进服务质量。研究选择了零售服务为试点,给管理人员提供了一个更直接、更清晰的指引,发挥人力资源本身的素质。研究结果把希士杰等质量大师在美国哈佛商报中提出的“服务利润连接（Ｓｅｒｖｉｃｅｐｒｏｆｉｔｃｈａｉｎ）”具体化,使管理人员可以直接在企业内运用。     

磁-光/涡流成像技术的有限元分析

近年来迅速发展的磁－光成像（ＭＯＩ）技术使涡流检测技术得到了新的进展。本文运用磁－光／涡流成像的有限元模型对典型的飞机构件缺陷（如连接飞机表面两个铝层的紧固件下面的裂纹）进行模拟。模拟结果表明,其磁场垂直分量的变化对这种结构来说是相当灵敏的,采用ＭＯＩ技术可以用来探测隐藏在紧固件帽下面的缺陷。     

Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares

High-energy X-rays and ??-rays from solar flares were discovered just over fifty years ago. Since that time, the standard for the interpretation of spatially integrated flare X-ray spectra at energies above several tens of keV has been the collisional thick-target model. After the launch of the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) in early 2002, X-ray spectra and images have been of sufficient quality to allow a greater focus on the energetic electrons responsible for the X-ray emission, including their origin and their interactions with the flare plasma and magnetic field. The result has been new insights into the flaring process, as well as more quantitative models for both electron acceleration and propagation, and for the flare environment with which the electrons interact. In this article we review our current understanding of electron acceleration, energy loss, and propagation in flares. Implications of these new results for the collisional thick-target model, for general flare models, and for future flare studies are discussed.     

Characterization and Calibration of the CheMin Mineralogical Instrument on Mars Science Laboratory

A principal goal of the Mars Science Laboratory (MSL) rover Curiosity is to identify and characterize past habitable environments on Mars. Determination of the mineralogical and chemical composition of Martian rocks and soils constrains their formation and alteration pathways, providing information on climate and habitability through time. The CheMin X-ray diffraction (XRD) and X-ray fluorescence (XRF) instrument on MSL will return accurate mineralogical identifications and quantitative phase abundances for scooped soil samples and drilled rock powders collected at Gale Crater during Curiosity’s 1-Mars-year nominal mission. The instrument has a Co X-ray source and a cooled charge-coupled device (CCD) detector arranged in transmission geometry with the sample. CheMin’s angular range of 5^° to 50^° 2θ with <0.35^° 2θ resolution is sufficient to identify and quantify virtually all minerals. CheMin’s XRF requirement was descoped for technical and budgetary reasons. However, X-ray energy discrimination is still required to separate Co?Kα from Co?Kβ and Fe?Kα photons. The X-ray energy-dispersive histograms (EDH) returned along with XRD for instrument evaluation should be useful in identifying elements Z>13 that are contained in the sample. The CheMin XRD is equipped with internal chemical and mineralogical standards and 27 reusable sample cells with either Mylar^? or Kapton^? windows to accommodate acidic-to-basic environmental conditions. The CheMin flight model (FM) instrument will be calibrated utilizing analyses of common samples against a demonstration-model (DM) instrument and CheMin-like laboratory instruments. The samples include phyllosilicate and sulfate minerals that are expected at Gale crater on the basis of remote sensing observations.