旋转光楔散斑照相术

本文提出了动态散斑照的一种新方法－旋转光楔散斑照相术，文中给出了理论分析及实验结果。该方法不仅能在一张记录介质上记录物体动变形的各状态的多通道散斑图，而且用全场滤波分析时，能方便地同时给出所有通道上的物体变形信息，得到清晰的、高衬比的干涉条纹图。这种方法是利用旋转光楔照相机来实现多通道动态散斑记录，具有设备简单、用途广泛等优点。文中给出了实测结果，理论分析与实验结果是吻合的。     

基于CATIA/CAA的快速布点技术研究

针对框、梁、壁板、翼肋、双曲面类机身蒙皮、模具型面等三坐标数字化测量前测量布点和数据准备效率低、布点规范性差和测量二维简图生成繁琐等问题,在典型测量特征的布点规则进行整理的基础上,提出了测量布点的算法.在CATIA的环境下,通过CAA二次开发,建立了测量布点平台,实现了框、梁、壁板、翼肋、双曲面类机身蒙皮、模具型面等零件测量点快速布置的功能,提高了测量点和数据的规范性,缩短了测量准备周期,在实际生产中有一定使用价值.     

非线性递推最小模型误差估计

基于最优控制理论和两点边值问题的不变式嵌入法，提出了模型不确定性非线性性系统递推最小模型误差估计，并推导了估计算法。仿真例说明，该方法是模型不确定性非线性系统状态递推估计的有效方法。     

用箭遥数据计算三轴稳定卫星初始姿态

在卫星发射中,利用星箭分离时刻的火箭遥测数据来确定卫星在入轨时的初始姿态,是主动段测控任务中准实时工作很重要的一环。文中从初始姿态确定的原理入手,对数据的选取和坐标系的定义进行描述,并对计算方法和步骤进行了讨论。通过实际应用,指出应注意的事项。     

三点法EST测量直线度的误差分析

叙述了三点法误差分离技术测量回转体素线直线度误差的原理，分析了参数选择、测头间距误差、传感器标定误差、工件安装误差对测量误差的影响，探讨了对信号谐波和测量噪声的抑制措施，以提高直线度误差的测量准确度。     

On the correlation of the solar wind observed at the L5 point and at the Earth

The L5 point is a promising location for forecasting co-rotating high-speed streams in the solar wind arriving at the Earth. We correlated the solar wind data obtained by the Nozomi spacecraft in interplanetary space and by the Advanced Composition Explorer (ACE) at the L1 point, and found that the correlation is significantly improved from that of the 27-day recurrence of ACE data. Based on the correlation between the two spacecraft observations, we estimated the correlation of the solar wind velocity between the L5 point and at the Earth, and found that the correlation coefficient was about 0.78 in late 1999, while that of the 27-day recurrence was 0.51. Eighty-eight percent of the velocity difference falls within 100 km/s between the L5 point and the Earth. This demonstrates the potential capability of solar wind monitoring at the L5 point to forecast the geomagnetic disturbances 4.5 days in advance.     

软件技术状态检查工具的研究

软件技术状态管理是保证软件技术状态的正确性、控制软件技术状态的不受控性、提高软件可靠性的有效技术保障 ,是软件质量管理的一个重要环节。本文简要介绍了该工具的开发背景、设计思想、功能、优点及应用前景     

导航星全球定位系统及其应用

较详细地介绍了导航星全球定位系统（ＧＰＳ）的组成、功能和发展过程。对该系统的导航定位原理、方法、精度度量方法，以及影响导航定位精度的误差进行了分析。全球定位系统是一个具有巨大的发展潜力和深透能力的系统，它的应用范围已超出了其原来的设计要求。最后还介绍了导航星全球定位系统的应用情况。     

Equilibrium positions on stationary orbits and planetary principal inertia axis orientations for the Solar System

We present a qualitative analysis in a phase space to determine the longitudinal equilibrium positions on the planetary stationary orbits by applying an analytical model that considers linear gravitational perturbations. We discuss how these longitudes are related with the orientation of the planetary principal inertia axes with respect to their Prime Meridians, and then we use this determination to derive their positions with respect to the International Celestial Reference Frame. Finally, a numerical analysis of the non-linear effects of the gravitational fields on the equilibrium point locations is developed and their correlation with gravity field anomalies shown.