一种改进的运动目标抗遮挡跟踪算法

为解决运动目标在遮挡情况下的跟踪问题,提出一种基于目标运动预测与自适应多子块模板匹配相结合的抗遮挡跟踪算法.该算法建立了多子块模板匹配相关算法中遮挡情况的判定、子块模板匹配及自适应更新等准则,采用卡尔曼滤波模型预测目标在遮挡时的运动轨迹,并利用一种基于目标速度矢量的模板定位规则实现目标在遮挡结束后的接力跟踪.将该算法应用于存在多种遮挡情况下的实际视频中进行测试,实验结果表明:该算法不仅能够实现在部分遮挡情况下的目标跟踪,而且能在严重遮挡、甚至完全遮挡情况下对刚体和非刚体目标进行稳定有效地跟踪,保持目标运动轨迹的可靠性和完整性.     

B737NG飞机反推系统故障分析

根据波音的相关技术文件,B737NG反推系统的部件有些本身带有设计缺陷或可靠性较低,导致反推系统故障较多。对反推系统的工作原理、常见故障及处理方法进行总结,使排故人员和故障管控工程师对该系统有深入的了解,方便大家开阔思路,减少排故的时间,提高排故效率。     

A novel cooperative mid-course guidance scheme for multiple intercepting missiles

In the interception engagement,if the target movement information is not accurate enough for the mid-course guidance of intercepting missiles,the interception mission may fail as a result of large handover errors.This paper proposes a novel cooperative mid-course guidance scheme for multiple missiles to intercept a target under the condition of large detection errors.Under this scheme,the launch and interception moments are staggered for different missiles.The earlier launched missiles can obtain a relatively accurate detection to the target during their terminal guidance,based on which the latter missiles are permitted to eliminate the handover error in the mid-course guidance.A significant merit of this scheme is that the available resources are fully exploited and less missiles are needed to achieve the interception mission.To this end,first,the design of cooperative handover parameters is formulated as an optimization problem.Then,an algorithm based on Monte Carlo sampling and stochastic approximation is proposed to solve this optimization problem,and the convergence of the algorithm is proved as well.Finally,simulation experiments are carried out to validate the effectiveness of the proposed cooperative scheme and algorithm.     

基于节点电压增量方程的电路故障子网络诊断

基于节点电压增量方程的电路故障诊断方法通常用来诊断线性电路中的元器件级的故障情况.本文将其推广应用于诊断大规模线性模拟电路中子网络级故障以简化测前仿真,提高诊断效率.     

相同设备在不同试验条件下试验图谱选择方法

同一机载设备可能安装在同一飞机的不同位置,而不同位置可能具有不同振动试验要求。为合理选择典型振动试验条件,使同状态机载设备既能经受考核验证又能满足产品互换性要求,以累计疲劳损伤理论为基础,以仿真为手段,以试验为验证,研究了不同试验条件对产品寿命的影响,并以产品寿命为依据,得出了试验条件的选择方法。     

防空导弹弹性振动抑制

基于防空导弹的数学模型,根据弹体弹性振动的特性,对抑制其振动的方法和稳定回路设计进行了研究。通过确定频带宽度稳定刚性弹体的姿态运动,采用陷波补偿相位稳定和增益稳定抑制弹性振动以稳定弹性弹体。给出了稳定回路的设计,并比较了不同方法的特点。     

基于自抗扰控制的导弹三维制导规律

针对导弹制导系统中存在模型不确定性和外部扰动的特点,提出了利用自抗扰控制器设计导弹三维制导规律的新方法.在建立导弹三维制导模型的基础上,把系统非线性部分、回路间耦合项以及目标机动加速度视为对制导系统的未知总扰动,从而将模型变换为适于自抗扰控制的仿射系统.通过为俯仰和偏航回路分别引入自抗扰控制器,实现了双回路的动态解耦,...     

一种基于火箭橇轨道的动基座重力 测量系统评价方法

传统的重力仪精度评价方法为重力仪测量值与静态定点值或飞行状态下的重力线网格参考值进行比较,根据差值或相对异常值来评价重力仪的精度指标,但其缺点是飞行轨迹重复性差.火箭橇轨道是进行火箭橇测试的重要组成部分,它严格按照设计建设,长达数公里,拥有完整已知的地理数据信息,且沿着火箭橇轨道布有众多的绝对重力基准点.提出一种基于火箭橇轨道的重力测量系统评价方法,通过火箭橇轨道上的众多绝对重力基准点和重力仪测量得到的重力值比较,评价重力仪的精度指标性能.其优点是该方法能够连续、快速、可重复评价重力测量系统的精度指标,为重力仪研制提供精确的评价手段和鉴定方法.     

The James Webb Space Telescope

The James Webb Space Telescope (JWST) is a large (6.6 m), cold (<50 K), infrared (IR)-optimized space observatory that will be launched early in the next decade into orbit around the second Earth–Sun Lagrange point. The observatory will have four instruments: a near-IR camera, a near-IR multiobject spectrograph, and a tunable filter imager will cover the wavelength range, 0.6 < ; < 5.0 μ m, while the mid-IR instrument will do both imaging and spectroscopy from 5.0 < ; < 29 μ m.The JWST science goals are divided into four themes. The key objective of The End of the Dark Ages: First Light and Reionization theme is to identify the first luminous sources to form and to determine the ionization history of the early universe. The key objective of The Assembly of Galaxies theme is to determine how galaxies and the dark matter, gas, stars, metals, morphological structures, and active nuclei within them evolved from the epoch of reionization to the present day. The key objective of The Birth of Stars and Protoplanetary Systems theme is to unravel the birth and early evolution of stars, from infall on to dust-enshrouded protostars to the genesis of planetary systems. The key objective of the Planetary Systems and the Origins of Life theme is to determine the physical and chemical properties of planetary systems including our own, and investigate the potential for the origins of life in those systems. Within these themes and objectives, we have derived representative astronomical observations.To enable these observations, JWST consists of a telescope, an instrument package, a spacecraft, and a sunshield. The telescope consists of 18 beryllium segments, some of which are deployed. The segments will be brought into optical alignment on-orbit through a process of periodic wavefront sensing and control. The instrument package contains the four science instruments and a fine guidance sensor. The spacecraft provides pointing, orbit maintenance, and communications. The sunshield provides passive thermal control. The JWST operations plan is based on that used for previous space observatories, and the majority of JWST observing time will be allocated to the international astronomical community through annual peer-reviewed proposal opportunities.