不确定混沌系统的变论域直接自适应模糊滑模控制

提出了一种用于不确定混沌系统的变论域自学习模糊滑模控制方法.引入变论域自适应模糊控制器逼近滑模控制的等效控制,消除因系统不确定性及干扰导致的等效控制无法准确确定,同时使控制器设计不依赖被控对象的精确数学模型.基于李雅普诺夫函数给出规则参数调整的自适应率,并确定滑模切换控制项以保证闭环控制系统的稳定性.根据滑模控制原理给出4条模糊规则以平滑不连续控制,实现高烦抖振削弱.某Lorenz混沌系统控制仿真结果表明:该法对系统参数突变和外部干扰具强鲁棒性,同时削弱了抖振.     

High resolution science with high redshift galaxies

We summarize the high-resolution science that has been done on high redshift galaxies with Adaptive Optics (AO) on the world’s largest ground-based facilities and with the Hubble Space Telescope (HST). These facilities complement each other. Ground-based AO provides better light gathering power and in principle better resolution than HST, giving it the edge in high spatial resolution imaging and high resolution spectroscopy. HST produces higher quality, more stable PSF’s over larger field-of-views in a much darker sky-background than ground-based AO, and yields deeper wide-field images and low-resolution spectra than the ground. Faint galaxies have steadily decreasing sizes at fainter fluxes and higher redshifts, reflecting the hierarchical formation of galaxies over cosmic time. HST has imaged this process in great structural detail to z  6, and ground-based AO and spectroscopy has provided measurements of their masses and other physical properties with cosmic time. Last, we review how the 6.5 m James Webb Space Telescope (JWST) will measure First Light, reionization, and galaxy assembly in the near–mid-IR after 2013.     

Semi-analytical investigations of high area-to-mass ratio geosynchronous space debris including Earth’s shadowing effects

This paper investigates the long-term perturbations of the orbits of geosynchronous space debris influenced by direct radiation pressure including the Earth’s shadowing effects. For this purpose, we propose an extension of our homemade semi-analytical theory [Valk, S., Lemaître, A., Deleflie, F. Semi-analytical theory of mean orbital motion for geosynchronous space debris under gravitational influence. Adv. Space Res., submitted for publication], based on the method developed by Aksnes [Aksnes, K. Short-period and long-period perturbations of a spherical satellite due to direct solar radiation. Celest. Mech. Dyn. Astron. 13, 89–104, 1976] and generalized into a more convenient non-singular formalism. The perturbations accounting for the direct radiation pressure with the Earth’s shadow are computed on a revolution-by-revolution basis, retaining the original osculating Hamiltonian disturbing function. In this framework, we compute the non-singular mean longitude at shadow entry and shadow exit at every orbital revolution in opposition to classical approaches where the singular eccentric anomalies at shadow entry and shadow exit are computed. This new algorithm is developed using non-singular variables. Consequently, it is particularly suitable for both near-circular and near-equatorial orbits as well as orbits which transit periodically around null eccentricities and null inclinations.The algorithm is tested by means of numerical integrations of the equations, averaged over the short periods, including radiation pressure, J₂, the combined Moon and Sun third body attraction as well as the long-term effects of the 1:1 resonance occurring for geosynchronous objects. As an extension of [Valk, S., Lemaître, A., Anselmo, L. Analytical and semi-analytical investigations of geosynchronous space debris with high area-to-mass ratios influenced by solar radiation pressure. Adv. Space Res., doi:10.1016/j.asr.2007.10.025, 2007b], we especially apply our analysis to space debris with area-to-mass as high as 20 m²/kg. This paper provides numerical and semi-analytical investigations leading to a deep understanding of the long-term evolution of the semi-major axis. Finally, these semi-analytical investigations are compared with accurate numerical integrations of the osculating equations of motion over time scales as high as 25 years.     

新型S波段宽频微带天线阵研究

微带天线是一种小型化、低剖面、可共形天线,研究了采用双层双排平行放置贴 片形式的二元微带贴片天线阵,通过缝隙耦合的馈电形式,可实现S波段宽频带通信技术要 求。给出了此类天线的设计方法,讨论了基片厚度对天线辐射特性的影响;通过基于时域有 限积分法的CST软件包仿真计算,得到该天线端口反射系数小于-10dB（VSWR<2）的相对带宽 为24％,满意的方向图带宽和增益特性,理论计算结果与实测值保持一致,验证了这种结 构天线较好的实际应用性能。     

基于支撑矢量机的织物疵点识别方法

为了对种类繁多的织物疵点使用机器进行有效的检测和分类,提出了基于直方图统计和支撑矢量机的织物疵点识别算法。该算法运用直方图统计的方法,由概率统计生成直方波形,并将其作为支撑矢量机的输入参数,用于训练特征样本集,以获得支撑矢量。实验表明,该算法用于织物疵点检测是可行、有效的,可得到满意的识别结果。     

同温层气球平台反向定位系统的研究

反向定位系统是针对驻留型同温层气球平台的一种新型定位系统 ,该系统的基本原理是由接收站的位置计算得出发射机的位置。文章采用卡尔曼滤波的方法 ,建立了反向定位系统的模型 ,给出其滤波算法 ;鉴于地面接收站的位置选择对该系统的定位精度有较大的影响 ,给出地面站选址依据 ,并通过计算、仿真获得一组较为理想的布站方式。此外 ,钟差是系统的一个主要误差源 ,文中对其引起的定位误差进行了分析 ,并给出估算的方法 ;对系统中的传播误差、设备误差也进行了分析。最后 ,对系统建立了仿真模型进行仿真。结果表明 ,该定位系统具有较好的定位精度     

光纤彩色三维图像实时全光传感器

对传像光纤的分辨率进行了研究,针对其出现的问题提出解决对策,并介绍了光纤彩色三维图像实时全光传感器的工作原理与实验结果,得出了以中性光子完全代替电子为信息载体的光纤彩色三维图像传感器,具有实时摄取、传递和显现立体彩色目标功能的结论.其抗电磁干扰与自隐身性极佳,在电子战争中或断电紧急时刻将成为机载影像电系统的后备补充.     

三维机翼亚临界定常流的局部线性化有限元法

本文使用了两种类型等参元,通过变分法,计算了三维机翼亚临界定常位势流中的压力分布,计算结果与试验结果符合较好。文中还使用了有限元法中的局部线性化理论,插值出元素中心点密度去处理迭代过程中元素系数阵的计算,其结果与通常的有限元计算相吻合,但计算时间却明显减少了。文中还对有限元法局部线性化理论和局部线性化有限元法做了阐述。     

飞机强度试飞活动部件残余变形分析

试飞中,飞机残余变形测量结果分析主要是判别所测残余变形是否为危及飞行安全、有碍操纵等的有害变形。而飞机活动部件残余变形实测结果常常超差的一个重要原因,是实际测量中,部件所处的状态与图纸要求的差异（存在偏度）。对此提出了偏度修正法和空间基准面修正法,并利用某型飞机全动平尾残余变形的实测数据,验证了这两种方法的有效性,并就方法的适用性进行了讨论。     

Time delay compensation in lateral-directional flight control systems at high angles of attack

The previous studies of time delay compensation in flight control systems are all based on the conventional aerodynamic derivative model and conducted in longitudinal motions at low angles of attack. In this investigation, the effects of time delay on the lateral-directional stability augmentation system in high-α regime are discussed based on the $\dot{\beta }$ model, which is proposed in our previous work and proved as a more accurate aerodynamic model to reveal the lateral-directional unsteady aerodynamic characteristics at high angles of attack. Both the $\dot{\beta }$ model and the quasi-steady model are used for simulating the effects of time delay on the flying qualities in high-α maneuvers. The comparison between the simulation results shows that the flying qualities are much more sensitive to the mismatch of feedback gains than the state errors caused by time delay. Then a typical adaptive controller based on the conventional dynamic derivative model and a gain-prediction compensator based on $\dot{\beta }$ model are designed to address the time delay in different maneuvers. The simulation results show that the gain-prediction compensator is much simpler and more efficient at high angles of attack. Finally, the gain-prediction compensator is combined with a linearized $\dot{\beta }$ model reference adaptive controller to compensate the adverse effects of very large time delay, which exhibits excellent performance when addressing the extreme conditions at high angles of attack.