角位移传感器校准方法及不确定度分析

描述了角位移传感器的迟滞、重复性、非线性等主要技术指标的校准方法、校准步骤和数据处理方法、测量不确定度评定方法。     

承力操纵装置性能试验台系统方案设计

介绍了一个飞机承力操纵装置性能试验台的实现机理、采用的方案,有助于增加读者对液压系统、液压性能试验台及液压伺服控制系统的了解。     

薄膜温度传感器的研制及应用

一种新型的薄膜温度传感器,采用真空镀膜的方法制作在涡轮叶片表面,两者构成一体,可以真实反应表面温度。传感器的质量小、响应快,对叶片内部换热和表面燃气流无干扰。 传感器的敏感元件为铂姥_(10)-铂热电偶,测温上限可达1000℃,测量精度为±3％。     

耐高温聚苯硫醚复合涂层性能的研究

主要讨论增韧材料对PPS性能的影响和各种填料用量对PPS复合涂层的附着力、抗冲击强度等性能的影响以及PPS复合涂层的耐高温性能。结果表明：增韧树脂PEK－C的加入可提高PPS共混树脂的力学性能；共混树脂中加入5％的石墨、10％TiO2时，可获得综合性能良好的复合涂层。     

C/C复合材料1 800℃抗氧化涂层探索研究

提出并制备了可以应用于1 800℃的抗氧化涂层体系,固渗法制备SiC内层,料浆涂刷法制备高温氧化物釉层和硼硅化物釉层.经扫描电镜分析涂层形貌及电子能谱分析其组成,发现C/C复合材料基材结构完整,没有发生次表面氧化.试验结果表明氧乙炔焰烧蚀20 s后,失重为0.06%;1 800℃自然对流氧化试验条件下,氧化物釉层30 min的平均失重速率为0.06g/(m2·s);硼硅化物釉层60min的平均失重速率为0.2g/(m2·s).说明涂层体系在1 800℃具有良好的抗氧化能力.     

The Cassini Cosmic Dust Analyzer

The Cassini-Huygens Cosmic Dust Analyzer (CDA) is intended to provide direct observations of dust grains with masses between 10⁻¹⁹ and 10⁻⁹ kg in interplanetary space and in the jovian and saturnian systems, to investigate their physical, chemical and dynamical properties as functions of the distances to the Sun, to Jupiter and to Saturn and its satellites and rings, to study their interaction with the saturnian rings, satellites and magnetosphere. Chemical composition of interplanetary meteoroids will be compared with asteroidal and cometary dust, as well as with Saturn dust, ejecta from rings and satellites. Ring and satellites phenomena which might be effects of meteoroid impacts will be compared with the interplanetary dust environment. Electrical charges of particulate matter in the magnetosphere and its consequences will be studied, e.g. the effects of the ambient plasma and the magnetic field on the trajectories of dust particles as well as fragmentation of particles due to electrostatic disruption.The investigation will be performed with an instrument that measures the mass, composition, electric charge, speed, and flight direction of individual dust particles. It is a highly reliable and versatile instrument with a mass sensitivity 10⁶ times higher than that of the Pioneer 10 and 11 dust detectors which measured dust in the saturnian system. The Cosmic Dust Analyzer has significant inheritance from former space instrumentation developed for the VEGA, Giotto, Galileo, and Ulysses missions. It will reliably measure impacts from as low as 1 impact per month up to 10⁴ impacts per second. The instrument weighs 17 kg and consumes 12 W, the integrated time-of-flight mass spectrometer has a mass resolution of up to 50. The nominal data transmission rate is 524 bits/s and varies between 50 and 4192 bps.This revised version was published online in July 2005 with a corrected cover date.     

红外隐身材料的现状与展望

综述了国内外红外隐身材料的发展历程，重点介绍了构成红外隐身材料的填料、树脂的研究现状以及近年来开始重点研究的红外兼容型多频谱隐身材料，并且指出了红外隐身材料的发展方向。     

金属板料单向拉伸引伸计及测试系统的研制

利用电阻应变式传感器的原理，研制了单向引伸计及测试系统，对金属薄料的成形性能参数应变刚指数n和厚向异性指数r进行检测，并成功地用于科研和教学活动中，在材料检测研究方面颇具价值。     

基于Riccati方程的离散容错控制系统设计

基于离散系统的Ｒｉｃｃａｔｉ方程，提出一种对传感器失效具有完整性的离散控制系统的设计方法，给出了完整性设计方法的设计步骤，并用设计实例验证了该方法的有效性．该方法还可推广用于执行器失效的情况．     

基于模糊逻辑的航空发动机虚拟传感器

在双通道的发动机控制系统中，未超过故障阈值的传感器慢漂移故障难以隔离，且在故障检出前影响控制系统的反馈信号。引入机栽自校正实时模型作为第三通道的虚拟传感器，并提出模糊隶属度加权和动态阈值技术以获得可靠的传感器适应值，实现双余度系统中失效传感器的检测和隔离。仿真结果表明，这种方法能可靠地改进适应信号，将由于传感器故障引起的发动机控制系统扰动抑制到0．2％以内，并能避免失控。