强海杂波背景下目标检测方法综述

高频地波雷达被广泛应用于海面目标的检测,而由于海杂波的分布散射具有很强的动态特性,通常情况下成为了海面目标检测的主要干扰成分.因此,在强海杂波背景下进行目标检测的关键在于如何有效抑制海杂波.从循环对消、子空间分解、模型预测以及分形特征这几方面对海杂波抑制技术进行综述、分析和总结,为后续对海面目标检测提供参考.     

某导弹武器系统可靠性优化

给出了系统可靠性与费用的关系 ,建立了某导弹武器可靠性优化模型 ,用MonteCarlo方法解决了此问题。     

基于Matlab语言的系统可靠性仿真

Matlab是一种高性能数值计算语言 ,本文用Matlab语言编制系统可靠性仿真程序 ,并给出了具体实例。此方法比其他方法简单有效 ,可适用于复杂系统。     

一类滞后不确定相似组合系统的分散控制

本文给出了一个使滞后的相似组合大系统镇定的分散鲁棒控制器的设计方法。不确定性是时变的,是以不确定参数出现在每个子系统中,而存在于互联项中的不确定性假设可能知道它的边界,当系统具有某种特征时,简化了一般控制器的设计。     

A practical nonlinear robust control approach of electro-hydraulic load simulator

This paper studies a nonlinear robust control algorithm of the electro-hydraulic load simulator （EHLS）. The tracking performance of the EHLS is mainly limited by the actuator＇s motion disturbance, flow nonlinearity, and friction, etc. The developed controller is developed based on the nonlinear motion loading model. The problems of the actuator＇s disturbance and flow nonlinearity are considered. To address the friction problem, the friction model of the loading motor is identified experimentally. The friction disturbance is compensated using the obtained friction model. Therefore, this paper considers the main three factors comprehensively. The developed algorithm is easy to apply since the controller can be obtained just with one step back-stepping design. The stability of the developed algorithm is proven via Lyapunov analysis. Both co-simulation and experiments are performed to verify the effectiveness of this method.     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

90°强曲率弯管内三维湍流流场的数值分析

本文根据作者发展的一种能计算任意截面形状 90°弯管内三维不可压缩湍流流场的分析方法,利用作者实验的圆截面弯管数据 ( R_c/D=0.87)检验 k- ε双方程湍流模型预示强曲率三维湍流流场的精度。计算了 R_c/D=2.3的矩形截面和 R_c/D=0.87的圆截面 90°弯管,并将计算结果与相应实验数据进行了比较分析。结果表明,即使对曲率很强的弯管,吸力面 (内侧壁 )不出现二次流迁移所形成的低速区前,标准 k- ε双方程模型仍能较好地预示出平均速度场。      

某伺服实时控制软件SFMEA/SFTA

对某助推伺服控制软件开展失效模式影响分析(SystemFailureModeandEffectsAnalysis,SFMEA) 和故障树分析(SoftwareFailureTreeAnalysis,SFTA)。SFMEA 是一种自下而上的分析方法,用以辨识出一系列可能的软件潜在故障模式,并评估其对系统工作的危害性。SFTA 是一种自上而下的分析方法,其目标是识别出基本事件(底事件),而基本事件可导致系统产生其所不希望发生的顶事件。应用SFMEA和SFTA的主要目的是提高软件和系统的安全性及可靠性。     

基于解调分选的时分多址信号时/频差参数联合估计方法

针对TDMA多时隙信号不连续,通信时隙外噪声以及其它用户信号影响时/频差参数估计的问题,首先证明了多时隙多普勒频差信号具有相参性,指出多时隙信号在相关处理中能量是可以积累的;在此基础上,根据通信时隙外噪声、其它用户信号与特定用户信号在时域上的可分离特性,提出基于解调分选的TDMA时/频差参数估计方法,并推导分析了该方法的处理性能。试验结果表明,提出的方法可以实现TDMA信号中多用户信号的时/频差参数联合估计,可以有效降低通信时隙外噪声与其它用户信号对参数估计精度的影响。     

液体火箭发动机热力组件动力学模型

 为了评判不同假设条件下得出的几种热力组件动力学模型的特点和适用范围,对其频率特性进行分析,并探讨了主要参数的影响规律。对于双组元非等温燃气流,在低频范围内采用考虑熵波效应的绝热流动模型更加精确。燃烧温度与混合比关系的无量纲斜率值越大,推进剂流量波动产生的熵波影响越明显。通过在分布参数流动模型中添加指数衰减率来表示熵波随频率的增大而耗散。改进的声学模型形式简单,既能在低频范围内描述熵波,又能在高频范围表征熵波的耗散,可以在很宽的频率范围内合理地描述燃气流动的动态特性。