基于合作目标的三维空间贝叶斯传感器配准算法

当存在合作目标时,基于合作目标的传感器配准算法往往优于基于多站测量的传感器配准算法.传统的基于合作目标的传感器配准算法将系统误差看作是一个确定未知量,对未知量的估计采用了非贝叶斯的参数估计算法,如极大似然法、最小二乘法等.当传感器量测噪声相对于传感器系统误差不可忽略时,上述算法估计效果较差.在此背景下,提出了基于合作目标的贝叶斯传感器配准算法,通过将传感器系统误差建模成未知的随机过程,并通过卡尔曼滤波消除量测噪声对系统误差估计带来的影响,实验结果表明,方法具有较好的实用性.     

带落角和末端攻角约束的最优末制导律

针对现代导弹武器多约束、高精度制导的基本要求,在综合考虑带落角和末端攻角约束的条件下,用二次型最优控制推导出一种新的最优末制导律。仿真结果表明,该末制导律既能够满足高精度制导的要求,同时也能够满足对落角和末端攻角的控制要求。     

海洋浊度测量传感器校准方法及校准测量能力评估

为了对海洋浊度测量传感器的计量性能做出快速、准确、科学的评价,构建了海洋浊度测量传感器的校准系统。本文详细阐述了海洋浊度测量传感器的校准原理,最佳校准方法的确立,并以具体实例介绍了校准数据处理及测量不确定度的评定,最后评估了该项目的校准测量能力(CMC),选用单一的相对值表示CMC,为2%。     

力臂自动调节装置智能综合测试系统的设计

为了解决力臂自动调节装置型号多、测试方法繁杂、测试精度低的问题,研制了以工控机为核心的自动测试系统,从硬件设计、软件设计入手,分析了测试过程中的工作环境模拟仿真与自动加载、系统控制信号和数据的共享、大气参数的测量、力臂值随机快速精确测量及抗干扰设计等问题,对改善力臂自动调节装置的维护手段、提高测试设备的自动化程度、使检测设备向综合化和智能化方向发展,具有重要的推动作用。     

扫描器运动多参数测试技术研究

新型图像扫描器具有较高的响应频率，可以实现高速扫描。在研究扫描器运动参数分离的基础上，利用对称放置的半导体位置探测器建立了扫描器的多运动参数测试系统，提出了光电二维位置传感器的非线性修正和补充方法，实现了四路模拟信号的DMA传送，提高了测试的速度和精度，实现扫描器在高频运动时的多运动参数测试。     

非线性传感器静态特性评估的极限点法

基于对测量过程、测量误差的认识，提出了一种利用极限点法评估非线性传感器静态特性的一种新方法。给出了利用该方法评估非线性传感器的两种模型。并以一电涡流式非线性位移传感器的标定数据进行了计算、分析。     

STUDY ON ALGORITHM OF SENSOR MANAGEMENT BASED ON FUNCTIONS OF EFFICIENCY AND WASTE

The sensor management system is a subsys-tem of a multisensor data fusion system,and itspurpose is to satisfy requests of multitarget andscanned space by using the limited sensor resourcesin order to gain optimal measurement values of allspecified characteristics ( detection and captureprobability,emission power of sensor,trackingprecision or target losing probability and so on) .By the optimal principle listed above,sensor re-sources are distributed in science and reason.In aword,itis a key p…     

Al-0.27Zr-0.064B实验合金的设计、熔炼及其变形特征

为研究等截面通道角形挤压过程中超细晶粒结构形成的机理及晶界变化过程 ,专门设计并熔铸了含微量Zr和B元素的Al 0 .2 7wt %Zr 0 .0 6 4wt%B合金 ,合金晶界上分布有大量的B2 Zr细小化合物颗粒 ,晶内几乎没有B2 Zr粒子。通过室温轧制、热锻以及随后的退火实验表明 ,B2 Zr具有很高稳定性 ,且再结晶后B2 Zr仍位于原变形后的位置 ,不随退火再结晶时新形成晶界的迁移而迁移 ,证明该合金可用于塑性变形时晶粒变形细化及晶界变化过程的研究     

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.     

燃气涡轮发动机地面试验传感器数据确认概念与方法研究

本文介绍了燃气涡轮发动机传感器数据确认系统的研究与应用现状,详细阐述了基于发动机和试验系统物理模型的解析冗余检验相关多传感器信号有效性方法,以及基于信号序列统计与时频特征分析的单传感器通道信号有效性的确认方法,提出了传感器数据有效性确认系统的研究框架。