激光外差干涉仪光电信号处理方法及特点

叙述和分析了外差激光干涉光电信号处理主其特点，指出了它们各自的应用范围，同时介绍了一处新型的光电信号处理方法，它不仅使外差干涉仪用于动态测量，而且可以同时实现高分辩率测量 。     

复杂系统的可靠性分析方法研究

本文对未来的运载器的复杂控制系统的可靠性建模、分配和预计的一般方法和程序及综合分析方法进行了讨论和研究。并简述了复杂系统的计算机辅助可靠性分析。     

Implementation of a three-phase high-power-factor rectifier with NPC topology

A three-phase four-wire power factor corrector based on neutral-point-clamped (NPC) topology is adopted to reduce the current harmonics and increase the input power factor. Using the NPC topology, the voltage stress of power switches can be reduced to the half of the dc-link voltage. With the dc-link voltage controller and the phase locked loop circuit, the balanced and sinusoidal line currents can be drawn from the ac supply system under the balance and unbalance mains voltages. The hysteresis current comparators are adopted in the current control loop to track the line current commands. Three voltage levels are generated on the ac terminal to the neutral point. Simulations and experiments are provided to verify the validity and the effectiveness of the proposed control scheme.     

航天遥感仪器的反射镜轻量化的研究

反射镜轻量化是航天遥感仪器轻型化的重要技术途径之一。阐述了反射镜轻量化的意义,反射镜材料的选择,玻璃反射镜轻量化的结构型式和设计要求、设计方案和计算以及温度试验结果。     

基于仿真的单元化制造系统的单元分组

在传统单元分组方法的基础上,提出了用仿真方法解决瓶颈机床的分组问题.采用着色Petri网,对生产系统建模.以BEA算法作为分组基础,经过仿真试验得到最终的单元分组结果.试验表明,用仿真的方法能够弥补传统分组算法复杂的缺点.     

一种无塔校准方法研究

在地面卫星测控系统中,目前使用较多的有塔校准技术具有一定的局限性,为了克服这种局限性,本文针对已有的卫星测控系统设备提出一种无塔校准方法,给出了具体无塔校相和无塔校零的实现方法.     

炉渣滤床技术处理亚麻生产废水

为了确定处理包头亚麻厂亚麻生产废水的设计方案，设计之前在现场进行了生产试验。在包头亚麻厂污水处理站，模拟炉渣滤床制造了3米高的炉渣滤层，滤渣从工厂锅炉房取用，将实际排放的亚麻煮漂车间、细纱车间、粗纱车间的生产废水混合后，通过炉渣滤层过滤处理，处理后出水由厂化验室和包头环保局化验。试验结果表明，处理后的排水各项指标完全达到国家排放标准。该工艺处理费用低，运行效果稳定，管理简便，具有明显的经济效益、环境效益和社会效益。     

基于特征模型的全系数自适应控制系统稳定性研究

讨论了基于特征模型的黄金分割加逻辑微分自适应控制律组成闭环系统的稳定性问题。针对参数未知、线性定常或慢时变的二阶不稳定对象,本文给出了在采样周期满足一定条件下,上述闭环系统渐近稳定的充分条件,其中包含对于时变参数变化范围和非线性阻尼系数的约束条件。     

Earthshine and Asteroseismology Telescope (East) Network

Several automated optical telescopes have been setup at appropriate longitudes around the globe to study earthshine variations and asteroseismology. The first telescope has been setup at Teide Observatory, Tenerife, Spain in October 2004. The intensity of earthshine relates to the average of Earth’s albedo, and in turn relates to the global temperature of the Earth. A global network is necessary because each site can measure the earthshine reflected from only a part of the Earth. The network will also be used for asteroseismology study. It can measure photometric variations of pulsating stars. The long-term and continuous measurements allow the accurate determination of mode frequencies of stellar pulsations, which provides information on the properties of stellar interior.