一种非线性系统集员辨识算法

针对带有未知有界噪声的非线性动态系统的鲁棒辨识问题,提出了一种新的非线性动态系统的集员辨识算法.利用径向基函数神经网络的逼近能力,根据系统的输入输出数据,选用径向基函数神经网络对未知非线性系统建模.径向基函数神经网络的中心被确定之后,考虑到建模误差与系统噪声有界,利用径向基函数神经网络为参数线性模型的特点,使用参数线性集员辨识算法辨识径向基函数神经网络的输出权值.由于集员辨识算法所得到的是网络输出权值的集合估计,在系统运行过程中,可以很方便地利用所建模型预测实际系统的输出范围.仿真表明,集员辨识算法辨识网络的输出权值比最小二乘法较少的受未知动态系统噪声分布的影响.     

Euler方程无网格算法及布点技术

研究了Bitina的显式无网格算法。在该算法的基础上,给出了Euler方程无网格离散形式,运用RungeKutta显式时间推进格式推进求解。文中的耗散项采用了与非结构网格上类似的守恒型耗散算子,边界条件的处理借鉴了结构化网格处理技术。此外,本文还描述了一种区域离散布点方法,研究了点云生成的选点准则,并成功地数值模拟了二维翼型的典型绕流。     

Orientations of LASCO Halo CMEs and their connection to the flux rope structure of interplanetary CMEs

Coronal mass ejections (CMEs) observed near the Sun via LASCO coronographic imaging are the most important solar drivers of geomagnetic storms. ICMEs, their interplanetary, near-Earth counterparts, can be detected in situ, for example, by the Wind and ACE spacecraft. An ICME usually exhibits a complex structure that very often includes a magnetic cloud (MC). They can be commonly modelled as magnetic flux ropes and there is observational evidence to expect that the orientation of a halo CME elongation corresponds to the orientation of the flux rope. In this study, we compare orientations of elongated CME halos and the corresponding MCs, measured by Wind and ACE spacecraft. We characterize the MC structures by using the Grad–Shafranov reconstruction technique and three MC fitting methods to obtain their axis directions. The CME tilt angles and MC fitted axis angles were compared without taking into account handedness of the underlying flux rope field and the polarity of its axial field. We report that for about 64% of CME–MC events, we found a good correspondence between the orientation angles implying that for the majority of interplanetary ejecta their orientations do not change significantly (less than 45 deg rotation) while travelling from the Sun to the near-Earth environment.     

基于Fuzzy理论的飞机故障诊断系统设计与实现

建立了某型飞机故障诊断的数学模型．开发了故障诊断系统的计算机软件．实现了以人机交互的方式在计算机上进行故障诊断，而且该诊断方法可以按飞机系统功能分解推广到各分系统。     

A statistical study of C IV regions in 20 Oe-stars

In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of absorption clouds and analyse their characteristics. From this analysis we can calculate the values of a group of physical parameters, such as the apparent rotational and radial velocities, the random velocities of the thermal motions of the ions, the Full Width at Half Maximum (FWHM), the optical depth, as well as the absorbed energy and the column density of the independent regions of matter, which produce the main and the satellite clouds of the studied spectral lines. Finally, we present the relations between these physical parameters and the spectral subtypes of the studied stars and we give our results about the structure of the C IV region in their atmosphere.     

数字全息测量超高速撞击碎片云实验研究

在中国空气动力研究与发展中心(CARDC)超高速碰撞中心(HIRC)7.6 mm超高速碰撞设备的基础上，搭建纳秒级脉冲激光数字全息系统。提出滤波片和衰减片组合布置，减弱超高速碰撞等离子体自发光、提高信噪比的方法。实验获得了2.25 mm铝球弹丸以4.0 km/s的速度撞击0.5 mm厚铝板形成碎片云的全息图。采用小波变换算法对碎片云全息图进行重建，得到超高速撞击碎片云的三维结构和碎片大小。碎片云的轮廓呈椭球型，分为碎片云的前端、核心和外壳，碎片主要分布在弹丸破碎形成的碎片云核心，存在大碎片，且分布较集中，对后板的损伤也严重     

PID控制器参数的隶属函数自整定技术及其应用研究

Ｐ Ｉ Ｄ 控制技术在工业过程控制中得到了广泛应用，但传统的 Ｐ Ｉ Ｄ 控制器不具有参数的在线整定功能，当系统工作条件较差时，难以满足控制要求，从而影响了控制品质的进一步提高。本文应用模糊数学中的隶属函数， 以工程施工机械中大量应用的液压阀控油缸为被控对象，建立数学模型和试验系统，实现 Ｐ Ｉ Ｄ 控制器参数的在线自整定。文中对其理论方法、计算机仿真和应用研究进行了论述。     

模糊数学在考试成绩分析中的应用

本文将模糊集合理论应用于考试分析，提出了一种对考试成绩的总体分布进行估计的较合理、有效的方法。     

Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.     

Coupled Clouds and Chemistry of the Giant Planets— A Case for Multiprobes

In seeking to understand the formation of the giant planets and the origin of their atmospheres, the heavy element abundance in well-mixed atmosphere is key. However, clouds come in the way. Thus, composition and condensation are intimately intertwined with the mystery of planetary formation and atmospheric origin. Clouds also provide important clues to dynamical processes in the atmosphere. In this chapter we discuss the thermochemical processes that determine the composition, structure, and characteristics of the Jovian clouds. We also discuss the significance of clouds in the big picture of the formation of giant planets and their atmospheres. We recommend multiprobes at all four giant planets in order to break new ground.