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.     

带有参考信号的直接序列扩频系统

扩频通信系统中码同步的精度及其电路的复杂程度直接影响系统的性能、体积和成本。采用发射参考信号法可以简化接收机端的码同步电路 ,从而大大减小遥控遥测系统及无线局域网中扩频接收机的体积和成本。本文给出了采用 MAXIM芯片组实现 UHF频段带有发射参考信号的直接序列扩频系统 ,并通过 System View软件进行了仿真 ,结果表明该方法可获得较好的通信性能 ,易于工程实现     

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.     

（20～400）MeV准单能中子参考辐射场的建立方法CSCD

为了满足对高能中子辐射场测量仪器进行校准的需要,必需建立20MeV以上的准单能中子参考辐射场.对国际上（20～400） MeV准单能中子参考辐射场的建立情况及建立方法进行了调研,可通过7Li（p,n）7Be反应获得该能区准单能中子场,中子束流轮廓可通过转换体和影像板进行测量,辐射场中子能谱可利用液体闪烁探测器或者238U裂变电离室通过飞行时间法进行测量,可建立高效率的反冲质子望远镜作为该能区的中子注量测量初级标准.     

Analysis of the DORIS contributions to ITRF2008

In its function as an ITRS Combination Centre, DGFI is in charge with the computation of an ITRF2008 solution. The computation methodology of DGFI is based on the combination of datum-free normal equations (weekly or session data sets, respectively) of station positions and Earth orientation parameters (EOP) from the geodetic space techniques DORIS, GPS, SLR and VLBI. In this paper we focus on the DORIS part within the ITRF2008 computations. We present results obtained from the analysis of the DORIS time series for station positions, network translation and scale parameters, as well as for the terrestrial pole coordinates. The submissions to ITRF2008 benefit from improved analysis strategies of the seven contributing IDS analysis centres and from a combination of the weekly solutions of station positions and polar motion. The results show an improvement by a factor of two compared to past DORIS data submitted to ITRF2005, which has been evaluated by investigating the repeatabilities of position time series. The DORIS position time series were analysed w.r.t. discontinuities and other non-linear effects such as seasonal variations. About 40 discontinuities have been identified which have been compared with the results of an earlier study. Within the inter-technique combination we focus on the DORIS contribution to the integration of the different space geodetic observations and on a comparison of the geodetic local ties with the space geodetic solutions. Results are given for the 41 co-location sites between DORIS and GPS.     

试用暗物质理论解释惯性和惯性力的物理机制(上)

基于对暗物质的多年探讨,我们认为宇宙空间是具有质量、相对均匀、连续稳定和有相当弹性暗物质群体(DMG)的空间.自然、宇宙万物终生处于群体引力制约之中,它们因此也获得了相应的惯性.本文立足于上述的宇宙空间,借助宇宙学原理、马赫原理和爱因斯坦等效原理,提出了物质客体的惯性机制和被称为虚力的惯性力机制 同时本文也解读所有惯...