激光光散射法测定BAG分子量及其分子量分布

介绍了一种用于高能推进剂新型键合剂BAG分子量和分子量分布测定的激光光散射法。给出了该方法的实验原理、实验步骤。该法以合镍化钾的二甲基酰胺溶液溶剂和流动相，凝胶渗透色谱柱为分离体系，实验结果表明：准确度和精密度较好，可作为常规测定BAG分子量及其分布的方法。     

导弹质量矩控制技术发展综述

质量矩技术是近年来导弹控制领域研究的热点问题之一。它是通过调整弹体内部活动质 量块的状态来实现导弹机动飞行的。与传统的气动舵控制方式相比,它具有响应快、气动外 形简单、无舵面烧蚀问题等优点,在大气层内高超声速飞行控制领域具有广阔的应用前景。 简述了质量矩技术的原理及应用领域,回顾了导弹质量矩控制技术的发展历程;从总体 布局、动力学建模、控制系统设计等方面综合分析了质量矩技术的研究现状;提出了一些当 前需要解决的难点问题,供相关人员参考。
     

无阻力卫星发展现状

以无阻力卫星的发展和相关技术为综述对象,首先介绍了无阻力卫星的概念,并比较无阻力卫星中位移模式和加速度计模式的区别和优缺点;其次分析了无阻力卫星的体系结构,将无阻力卫星控制系统分为无阻力控制回路、悬浮控制回路和卫星本体控制回路;然后描述了无阻力卫星中的检测质量、主要硬件的功能与特性,最后列出了无阻力卫星中主要的关键技术。     

非圆信号虚拟阵列波束形成算法

利用非圆信号的实值特性,提出了一种利用信号共轭扩展阵列孔径的虚拟阵列构成方法,将其应用在自适应波束形成中,对其波束形成的性能进行了分析和改进,并提出了一种快速的实现方法。该虚拟阵列的构造方法能同时保留时间信息和方位信息,用于自适应波束形成中,可以改善波束图形状,提高阵列增益,对抗超自由度干扰。计算机仿真验证了该方法的优越性。     

一种海洋测高卫星质心在轨估计算法

为了满足海洋测高卫星在轨质心位置精度的要求,提出了一种使用陀螺仪测量数据在轨估算卫星质心位置的算法。该算法利用推力器工作产生外力矩,采用总体最小二乘法,综合考虑了实际推力器推力的误差及陀螺仪的测量误差,由卫星的姿态动力学方程估算得到卫星质心位置。数值仿真证明了该算法的有效性,结果表明质心位置的估计精度在毫米量级,可以满足海洋测高卫星对质心位置精度的需求。     

基于虚拟仪器和PXI总线的电磁阀控制系统研制

为满足姿轨控火箭发动机快响应电磁阀的高精度脉冲控制需求,研制了一套基于虚拟仪器和PXI总线的脉冲控制系统。该系统选用成熟PXI总线硬件平台,设计可靠的电磁阀驱动电路,在LabVIEW图形化编程环境中完成控制软件的设计开发。经过全面的系统测试和验证后,控制系统多次应用于发动机地面试验中,表现出性能优良、可靠性高的特点,实现了快响应电磁阀的高精度脉冲控制。     

空间目标轨道信息软件平台的建设

空间目标轨道信息是空间态势感知的重要要素,是空间碰撞预警、空间碎片环境模型和许多空间应用的基础。因而,空间目标轨道确定成为空间态势感知的主要任务之一。文章介绍武汉大学测绘学院正在开发建设的空间目标轨道信息服务软件平台,该平台拥有的主要功能有:利用多源数据的卫星/空间碎片轨道确定(包括初轨确定)与预报、大气质量密度模型精化、空间碰撞预警和半解析法快速精密轨道传播等。文章还针对软件平台功能的研究进展进行了综述,介绍了软件平台发展规划。     

Learning relative directions between landmarks in a desktop virtual environment

This study presents two experiments that examine howindividuals learn relative directions betweenlandmarks in a desktop virtual environment. Subjectswere presented snapshot images of different virtualenvironments containing distinguishing landmarks anda road network. Following the presentation of eachvirtual environment, subjects were given a relativedirection test. The relative direction test involvedindicating the direction of hidden landmarks fromdifferent vantage points in the environment. Half ofthese vantage points were presented during thelearning phase, while the other half were novel.Results showed that subjects learned relativedirections between landmarks equally well when sceneswere presented in either a sequential or random order.Furthermore, viewing a configuration of landmarks ina desktop virtual environment from multipleperspectives produced a viewpoint dependentrepresentation in memory. Subjects had significantlygreater response times for new viewing perspectives,as compared to previously viewed scenes. Thisviewpoint dependent representation of the environmentpersisted despite learning under conditions ofspatio-temporal discontinuity and changes to anenvironmental frame of reference.     

SMESE (SMall Explorer for Solar Eruptions): A microsatellite mission with combined solar payload

The SMESE (SMall Explorer for Solar Eruptions) mission is a microsatellite proposed by France and China. The payload of SMESE consists of three packages: LYOT (a Lyman α imager and a Lyman α coronagraph), DESIR (an Infra-red Telescope working at 35–80 and 100–250 μm), and HEBS (a High Energy Burst Spectrometer working in X- and gamma-rays).     

Evolution of solar wind structures from 0.72 to 1 AU

Understanding the evolution of solar wind structures in the inner heliosphere as they approach the Earth is important to space weather prediction. From the in situ solar wind plasma and magnetic field measurements of Pioneer Venus Orbiter (PVO) at 0.72 AU (1979–1988), and of Wind/Advanced Composition Explorer (ACE) missions at 1 AU (1995–2004), we identify and characterize two major solar wind structures, stream interaction regions (SIRs) and interplanetary coronal mass ejections (ICMEs). The average percentage of SIRs occurring with shocks increases significantly from 3% to 24% as they evolve from 0.72 to 1 AU. The average occurrence rate, radial extent, and bulk velocity variation of SIRs do not change from 0.72 to 1 AU, while peak pressure and magnetic field strength both decrease with the radial evolution of SIRs. Within the 0.28 AU distance from the orbit of Venus to that of Earth, the average fraction of ICMEs with shocks increases from 49% to 66%, and the typical radial extent of ICMEs expands by about a fraction of 1.4, with peak pressure and magnetic field strength decreasing significantly. The mean occurrence rate and expansion velocity of ICMEs do not change from 0.72 to 1 AU.