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。      

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。     

基于星间测距的卫星自主导航中异常值剔除方法

在星间观测值数据传输中,由于种种因素有个别值与其他值截然不同,对定轨精度造成了严重的影响,必须对这些违反测量过程规律的异常测量值进行剔除。提出一种运用轨道积分器与设定随时间实时变化的门限值对星间距离观测值进行异常值剔除的方法。仿真结果表明,这种异常值剔除方法能够成功剔除观测误差大于等于180m的异常值,较精确、实时地剔除了对定轨结果影响较大的异常值,在卫星导航领域具有一定的应用价值。     

Lunar lander's three-dimensional translation and yaw rotation motion estimation during a descent phase using optical navigation

Optical navigation for a lunar lander consists of estimating a lander's 3-dimensional (3-D) relative dynamic motion with respect to a preselected landing site using a passive 2-dimensional (2-D) video image sequence. Lunar landing missions require a lander to perform an autonomous accurate landing with simple mechanical structure, easy operation and low cost. These requirements have motivated the need to develop an advanced navigation system. Existing navigation systems trade-off simplicity, accuracy and cost. High accuracy navigation systems typically imply complexity and high cost. In this paper, we consider a scenario where the descending phase starts from an initial altitude of 10 km with a time-of-descent of 100 s. The navigation camera is an off-the-shelf optical instrument used to take the video image sequence of the landing site during the landing phase. It is fed into the motion estimation algorithm to be processed. The continuous wavelet transform (CWT) is used to analyse each image frame of the input digital video image sequence. The output is a 2-D video image motion trajectory map, which represents the projection motion of the landing site. The 2-D video image motion is projected back to the 3-D lander's relative motion based on a geometric analysis. The outputs of this estimation algorithm are the 3-D attitude motion parameters of the lander at a time corresponding to an image being taken. The attitude determination and control system (ADCS) of the lander uses these data to perform the lander's attitude control task. In this article, we provide the motion modelling for a lunar lander during the descending phase. The projection of a 3-D planar to 2-D image plane is analysed which build the correspondence between the 3-D lander's motion and the 2-D image motion. This link provides the evidence for the geometry analysis. CWT is reviewed and CWT for video image sequence analysis is also introduced. Numerical simulation of the estimated 2-D video image sequence under the lander performing a 3-D translation and yaw rotation during the terminal descent are shown to verify the proposed concepts. The analysis of the results show that the proposed method achieves highly accurate 2-D video image motion estimation of less then 1% error with significant savings of cost, mass and volume. It leads to the accurate estimation of the lander's 3-D relative motion with respect to the landing site.