数字示波器测量幅度的误差分析

分析了用数字示波器测量脉冲幅度带来的测量误差,给出了计算相对误差的公式,对测量中产生的超差现象和异常现象的原因进行了分析.     

医学专家系统开发工具BFBEST的设计方法

本文详细描述了医学专家系统开发工具——BFBEST(Blackboard Framework Based Expert System Development Tool)设计方法和技术。包括知识获取方法和知识表示方法,推理机的设计,开发机的设计,以及系统解释功能与自学习功能的设计等。BFBEST是在IBMPC上采用Turbo-Prolog语言研制成功的。利用BFBEST能很方便地生成各种高性能的医学专家系统。     

Performance improvement of real-time PPP ambiguity resolution using a regional integer clock

Obtaining reliable GNSS uncalibrated phase delay (UPD) or integer clock products is the key to achieving ambiguity-fixed solutions for real-time (RT) precise point positioning (PPP) users. However, due to the influence of RT orbit errors, the quality of UPD/integer clock products estimated with a globally distributed GNSS network is difficult to ensure, thereby affecting the ambiguity resolution (AR) performance of RT-PPP. In this contribution, by fully utilising the consistency of orbital errors in regional GNSS network coverage areas, a method is proposed for estimating regional integer clock products to compensate for RT orbit errors. Based on Centre National d’Études Spatiales (CNES) RT precise products, the regional GPS/BDS integer clock was estimated with a CORS network in the west of China. Results showed that the difference between the estimated regional and CNES global integer clock/bias products was generally less than 5 cm for GPS, whereas clock differences of greater than 10 cm were observed for BDS due to the large RT orbit error. Compared with PPP using global integer clock/bias products, the AR performance of PPP using the regional integer clock was obviously improved for four rover stations. For single GPS, the horizontal and vertical accuracies of ambiguity-fixed PPP solutions were improved by 56.2% and 45.3% on average, respectively, whereas improvements of 67.5% and 50.5% in the horizontal and vertical directions, respectively, were observed for the combined GPS/BDS situation. Based on a regional integer clock, the RMS error of a kinematic ambiguity-fixed PPP solution in the horizontal direction could reach 0.5 cm. In terms of initialisation time, the average time to first fix (TTFF) in combined GPS/BDS PPP was shortened from 18.2 min to 12.7 min. In view of the high AR performance realised with the use of regional integer clocks, this method can be applied to scenarios that require high positioning accuracy, such as deformation monitoring.     

机械臂运动学建模及解算方法综述

以串联结构的机械臂为主要研究对象，首先调研了国内外机械臂正逆运动学建模及求解的主流方法，从数学工具、模型建立、求解手段等三个方面分析上述方法的基本原理，分析其优缺点。接着介绍了工程应用中解决机械臂运动学建模及求解问题所用的软件库，得到了不同软件库的精度和计算效率。最后提出了机械臂运动学建模及求解中存在的重要科学问题。通过总结上述方法，为研究人员在该领域内的理论研究及工程实现提供解决思路。     

小波变换在层板实时损伤检测中的应用

采用小波变换作为复合材料层合板损伤检测信号的分析工具,在获得复合材料层合板的动力学响应的基础上,应用小波分析工具对结构响应信号进行提取,对含噪声信号则先作降噪声处理,然后再进行小波分解,根据各种响应信号对损伤的灵敏度,选择损伤特征,通过捕捉结构出现损伤的时刻,实现复合材料损伤实时监控.      

区域观察小卫星星座重构方法研究

在对地观测任务中，经过优化设计的卫星星座通常具有较强的适应能力。但是，当星座中某颗卫星失效或地面需求发生变化时，就需要进行星座重构，以恢复或增强对部分地区的观察能力。提出了小卫星区域观察组网的方法，重点探讨了在应急情况下区域观察小卫星星座的重构问题，研究了节省能量的卫星轨道机动方法，特别提出了保持轨道属性和星座基本构形的预置量机动方法，分析了应急机动星座重构的几种情况，给出了每种情况的星座重构策略。     

基于力学特性预示的上面级结构改进设计

上面级结构复杂,各组件之间的刚度、质量差异很大,且飞行时处于高过载状态,如设计不合理,易产生局部模态和应力集中的问题,影响结构安全。应用PATRAN/NASTRAN软件系统进行上面级结构的力学特性预示,对出现的模态局部化和应力集中进行了分析,并提出改进设计方案,比较了改进设计前后的效果,改进后的模态和应力情况都得到明显改善。     

Protostellar Winds and Chondritic Meteorites

We discuss the interaction between the magnetosphere of a young star and its surrounding accretion disk. We consider how an X-wind can be driven magnetocentrifugally from the inner edge of the disk where accreting gas is diverted onto stellar field lines either to flow onto the Sun or to be flung outwards with the wind. The X-wind satisfies many observational tests concerning optical jets, Herbig-Haro objects, and molecular outflows. Connections may exist between primitive solar system materials and X-winds. Chondrules and calcium-aluminum-rich inclusions (CAIs) experienced short melting events uncharacteristic of the asteroid belt where meteorites originate. The inner edge of the solar nebula has the shortest orbital timescale available to the system, a few days. Protosolar flares introduce another timescale, tens of minutes to hours. CAIs may form when solids are lifted from shaded portions of the disk close to the Sun and are exposed to its intense light for a day or so before they are flung by the X-wind to much larger distances. Chondrules were melted, perhaps many times, by flares at larger distances from the Sun before being launched and annealed, but not remelted, in the X-wind. Aerodynamic sorting explains the narrow range of sizes with which CAIs and chondrules are found in chondritic meteorites. Flare-generated cosmic-rays may induce spallation reactions that produce some of the short-lived radioactivities associated with primitive solar system rocks. This revised version was published online in June 2006 with corrections to the Cover Date.     

云计算综述

论述了云计算的起源、概念、特点,与分布式计算和网格计算的区别;介绍了云计算厂商,及各厂商采用的数据存储、数据管理、编程模式、提供的服务种类云计算存在的问题,特别是云计算安全的风险种类及防护方法。提出了云计算需解决的问题。