机内测试虚警分析和控制

现代飞行器广泛采用机内测试(Built-intest,BIT)技术,以便对其内部故障进行自动检测、诊断和隔离,但是常规BIT面临诊断能力不足和诊断模糊性等问题,导致BIT虚警率高,难以有效发挥其应有的作用.本文论述了BIT虚警的基本理论、虚警的危害及现状,并从BIT虚警产生的原因分析入手,提出了解决虚警问题的一些方法和措施.     

某型飞机离子火警系统虚警故障分析及预防

针对某型飞机离子火警系统虚警故障,在分析故障原因的基础上,提出修理、维护等方面的预防改进措施,为飞机离子火警系统的修理提供借鉴。     

末制导雷达虚警概率检验方法

针对只有10^-8～10^-9量级的末制导雷达虚警概率难以检验的问题,研究虚警概率与发现概率、虚警时间的关系,论证了将虚警概率转化为虚警时间的检验方法,利用定时截尾统计检验理论,研究了不同鉴别比、不同试验时间、不同接收故障数时研制方与使用方的风险,提出了新型末制导雷达虚警概率的检验方法,解决了该项指标检验的难题。     

飞机电缆屏蔽典型工艺分析

简述了在飞机大修、改装和维护等工作过程中电缆所出现的一些应引起注意的工艺性问题,并通过一些故障照片加以说明,为飞机维护提供参考.     

基于一种灰色聚类滤波算法的飞机远程故障诊断虚警辨识方法

 在航线排故过程中,常会出现飞机远程实时故障报文信息的“飞机通信与寻址系统(ACARS)虚警”现象,使排故效率降低。对此,本文将灰色聚类和滤波理论结合提出了一种新的辨识算法——灰色聚类滤波算法,将常增益滤波引入灰色聚类算法,在灰色聚类算法中使用ACARS报文故障的当前数据分类故障、判断虚警的基础上,增加报文故障的历史数据,用滤波方法将历史的和当前的数据结合起来,提高辨识虚警的准确性。本算法应用于航空公司的波音777机队,能够有效辨识飞机实时故障报文信息中的虚警。     

某型雷达引信虚警分析与控制

针对某型雷达引信随机振动试验中虚警频发现象,从雷达引信工作原理、振动过程中虚警的产生机理出发,结合雷达引信的结构组成,分别从装配环节、低频电路分析、微波组件等方面分析了造成引信虚警的原因,并提出修理环节中解决并控制振动噪声的措施。     

某机载设备虚警问题的原因分析及处理方法

分析了外场试飞过程中某机载设备BIT虚警产生的原因及引起的后果,并提出了一套较为全面的BIT虚警解决方案,最后结合实际应用给出了便捷有效的软件算法实例。经过外场试飞验证,该算法大大降低了BIT虚警率,提高了设备的可靠性,并为同类型的机载设备产生的BIT虚警提供了可借鉴的经验。     

左起落架轮载开关线路故障的分析

通过排除一起典型电连接器和电缆安装质量问题,详细分析故障产生的原因,制定相应的维护措施,避免同类故障的再次发生。     

基于专家知识的故障诊断隔离系统研究

对试飞阶段外场维护故障信息进行提炼,建立了基于专家知识的飞机排故系统,节省排故时间,提高故障诊断效率。针对已有故障,分析同一故障描述下多种隔离方法无法选择的问题,提出了基于信息库的灰色关联优化模型。针对新兴故障无从下手、排故效率低、周期长的问题,建立了基于电子交互维护手册(IEMM)的故障诊断系统。本文故障诊断系统可保证维护人员在故障发生时更有效地分析故障原因、隔离方法,提高自主排故及外场维护能力。     

地线断路引起的ПНК系统综合性故障分析

一起ПНК导航驾驶综合系统信号地线电缆断线故障引起了三种故障现象,虽然故障不影响系统自检和一般性功能操作,但很容易被忽视。通过分析该故障产生的原因和机理,总结了日常维护与检查时应注意的事项。     

Low-Loss Almost Constant False-Alarm Rate Processors

Conventional normalizing constant false-alarm rate (CFAR) circuits use the same configurations when detecting targets in interference regions and in clear regions. The CFAR penalty incurred in the clear region can be reduced by using CFAR processors that recognize the region is clear so that normalization is not necessary. An analysis of the target-detection performance for a particular modified CFAR processor, for an active-radar sensor, and for a passive infrared (IR), or sonar, sensor is given. It is shown that the decreased CFAR penalty in the clear is coupled with an increase of false-alarm rate in the clutter regions.     

Minimal-Order Models for False-Alarm Calculations on Sliding Windows

A procedure is developed to obtain practical numerical results in connection with the m-out-of-n sliding-window detection problem. This effort was motivated by difficulties with previous approaches involving approximation, Markov models, and Monte Carlo simulation. Generating-function methods were found to be unsatisfactory for window lengths greater than 6 due to their complexity. Instead, a Markov model is described that is then constructively reduced to the minimum number of state variables. The results are derived for binary strings with intersymbol correlation. Computational aids are discussed for obtaining design information, such as quantiles, from the minimal-order Markov models. Numerical results are given comparing the methods of the paper with a "jumping" window approximation for an 8/10 problem.     

False-Alarm Regulation in Log-Normal and Weibull Clutter

Automatic detection radars require some method of adapting to variations in the background clutter in order to control their false-alarm rate. Conventional cell-averaging techniques designed to maintain a constant false-alarm rate in Rayleigh clutter will fail to control the false-alarm rate in more severe clutter environments such as log-normal or Weibull clutter. A processor is described which is capable of maintaining false-alarm regulation in log-normal clutter and in Weibull clutter (and, under certain conditions, over the entire family of log-normal and Weibull distributions).     

Adaptive Radar Detection with Asymptotically Regulated False-Alarm Rate

An adaptive detection procedure is described by which the detection threshold is so adjusted as to provide an asymptotic false-alarm probability PFA that is approximately invariant with changes in radar clutter return amplitude probability density functions (pdf's) in a broad class. The class includes Rayleigh, chi, Weibull, and lognormal pdf's. The receiver noise is also taken into account. The clutter-plus-noise pdf is approximated by a truncated generalized Laguerre series, the coefficients of which are estimated from the radar returns using "cell averaging" techniques. This estimation is assumed to be perfect. The results obtained indicate that the "bias" error, defined as the normalized difference between the design PFA and the asymptotic PFA corresponding to the computed threshold, lies within a fraction of an order of magnitude for 10-3?PFA ? 10-6. For PFA ?10-6 the bias error is more than an order of magnitude. These results are for the case when a single independent radar return is processed at a time. The bias error decreases as the number of postdetection integrations of independent returns increases.     

Magnetospheric Science Objectives of the <Emphasis Type="Italic">Juno</Emphasis> Mission

In July 2016, NASA’s Juno mission becomes the first spacecraft to enter polar orbit of Jupiter and venture deep into unexplored polar territories of the magnetosphere. Focusing on these polar regions, we review current understanding of the structure and dynamics of the magnetosphere and summarize the outstanding issues. The Juno mission profile involves (a) a several-week approach from the dawn side of Jupiter’s magnetosphere, with an orbit-insertion maneuver on July 6, 2016; (b) a 107-day capture orbit, also on the dawn flank; and (c) a series of thirty 11-day science orbits with the spacecraft flying over Jupiter’s poles and ducking under the radiation belts. We show how Juno’s view of the magnetosphere evolves over the year of science orbits. The Juno spacecraft carries a range of instruments that take particles and fields measurements, remote sensing observations of auroral emissions at UV, visible, IR and radio wavelengths, and detect microwave emission from Jupiter’s radiation belts. We summarize how these Juno measurements address issues of auroral processes, microphysical plasma physics, ionosphere-magnetosphere and satellite-magnetosphere coupling, sources and sinks of plasma, the radiation belts, and the dynamics of the outer magnetosphere. To reach Jupiter, the Juno spacecraft passed close to the Earth on October 9, 2013, gaining the necessary energy to get to Jupiter. The Earth flyby provided an opportunity to test Juno’s instrumentation as well as take scientific data in the terrestrial magnetosphere, in conjunction with ground-based and Earth-orbiting assets.     

Simulation of <Emphasis Type="Italic">Z</Emphasis>-crimp shaping with the use of the ansys finite element software

A finite element model of the Z-crimp shaping from a hard sheet blank is developed and a number of calculations using the ANSYS finite element software is conducted. The calculations are carried out in the framework of elastoplastic behavior of the blank material using the classical model of bilinear kinematic (translational) hardening with corresponding parameters of elasticity and plasticity. The model takes into account kinematics of spatial transformation of the shaping equipment as well as the time-variable conditions of its contact interaction with the blank.     

“Reinventing” career development

The following topics are dealt: career development definition; career development as a part of effective management; job satisfaction issues; motivated abilities; a case study results; identification of motivational patterns; and 'reinvention' of career development     

Comment on “Inversion of all principal submatrices of amatrix”

The paper by Koc and Chen (1994) includes new formulas for computational complexity, but the method itself is already known and has dubious numerical stability. A poorly conditioned example is shown