智能结构技术综述

对智能结构及其分类、技术基础、工作机理等,做了论述,阐述了智能结构技术现状和发展趋势。强调了主动结构的设计概念。指出智能结构的时代即将来临。     

基于Petri网的空中交通管制辅助决策系统

空中交通管制系统是生产实际中的一种典型的离散事件动态系统（Ｄｉｓｃｒｅｔｅ ｅｖｅｎｔ ｄｙｎａｍｉｃｓｙｓｔｅｍ,ＤＥＤＳ）,而Ｐｅｔｒｉ网理论是研究ＤＥＤＳ的有力工具之一。为了描述空中交通管制系统受到外部控制的交互机制及层次结构,文中引入Ｐｅｔｒｉ网概念的一类扩充－－开放Ｐｅｔｒｉ网的概念,并用开放Ｐｅｔｒｉ网工中交通管制辅助决策系统进行建模与分析,阐述了空中交通管制辅助决策系统的开放Ｐｅｔｒ     

CFRP管件的弯曲蠕变行为试验研究

为评价航天器结构中碳纤维增强树脂基(CFRP)复合材料管件的使用可靠性,开展了三点弯曲加载条件下CFRP管件弯曲性能和蠕变行为试验研究。进行了管件弯曲模量和弯曲强度测试、500 h时长的恒温蠕变测试以及–60℃~100℃和–160℃~80℃两种高低温循环蠕变测试,获得了典型温度工况、不同应力水平作用下管件弯曲蠕变变形规律。根据测试结果,确定了基于时间–温度–应力等效原理的管件蠕变主曲线以及唯象蠕变Findley模型,预测分析了管件长期蠕变变形;采用最大应变强度准则,对该CFRP管件的强度特性和安全承载能力进行了评价。结果表明,该CFRP管件在设计服役期限内能够满足蠕变变形与强度要求。     

TC-2型液压三轴飞行模拟转台伺服系统

飞行模拟转台(亦称动态角运动模拟器)是飞机和导弹飞行控制系统地面飞行仿真试验的关键设备之一。本文叙述了TC-2型液压三轴飞行模拟转台修改设计的指导思想和性能要求,介绍了转台伺服系统以及系统调试结果。最后,还介绍了该设备在飞行器控制系统地面物理仿真过程中实际使用的情况。     

ESPRIT算法在单快拍阵列信号中的应用

ESPRIT算法利用旋转不变技术估计信号参数,是近年来提出的阵列信号处理理论的一个新领域,它具有高分辨率、高精度、不需空间搜索等优点。单快拍总被当作相干信号处理,本文采用了Teoplitz结构协方差矩阵估计,起了空间平滑作用,所以可以估计相于信号源的波达方向(DOA),与标准空间平滑协方差矩阵估计相比较,Teoplitz协方差阵估计在总体上提高了信噪比,并且不牺牲阵列孔径。 计算机模拟结果表明,基于Teoplitz结构协方差矩阵的TLS-ESPRIT算法在20dB信噪比下,可以分辨出相隔0.2瑞利波束宽度的空间信号。     

空间实验室大面积太阳电池阵技术研究

介绍了空间实验室大面积太阳电池阵的方案构型，并进行了模态分析、热结构耦合分析和动力学仿真分析。生产出了全尺寸的集成演示样机，进行了展开试验、主展开机构的模态试验，以及半刚性太阳电池板和二自由度驱动机构的振动试验。计算和试验结果表明，技术方案是可行的。     

柔性多体撞击系统的精细H∞控制研究

本文在柔性多体撞击系统动力学方程的基础上 ,将撞击看成是一种扰动 ,设计了一个稳定的控制器以使撞击扰动对控制输出的影响达到最小的目的 ,在分析过程中采用 H∞ 控制原理对该问题进行了研究。在计算中 ,将精细积分法应用于状态动力学方程和 Riccati方程的求解中 ,使计算精度得到大幅度提高。最后通过数值例题说明了本文方法的有效性     

Nonclassical Transport and Particle-Field Coupling: from Laboratory Plasmas to the Solar Wind

Understanding transport of thermal and suprathermal particles is a fundamental issue in laboratory, solar-terrestrial, and astrophysical plasmas. For laboratory fusion experiments, confinement of particles and energy is essential for sustaining the plasma long enough to reach burning conditions. For solar wind and magnetospheric plasmas, transport properties determine the spatial and temporal distribution of energetic particles, which can be harmful for spacecraft functioning, as well as the entry of solar wind plasma into the magnetosphere. For astrophysical plasmas, transport properties determine the efficiency of particle acceleration processes and affect observable radiative signatures. In all cases, transport depends on the interaction of thermal and suprathermal particles with the electric and magnetic fluctuations in the plasma. Understanding transport therefore requires us to understand these interactions, which encompass a wide range of scales, from magnetohydrodynamic to kinetic scales, with larger scale structures also having a role. The wealth of transport studies during recent decades has shown the existence of a variety of regimes that differ from the classical quasilinear regime. In this paper we give an overview of nonclassical plasma transport regimes, discussing theoretical approaches to superdiffusive and subdiffusive transport, wave–particle interactions at microscopic kinetic scales, the influence of coherent structures and of avalanching transport, and the results of numerical simulations and experimental data analyses. Applications to laboratory plasmas and space plasmas are discussed.     

Volatile Trapping in Martian Clathrates

Thermodynamic conditions suggest that clathrates might exist on Mars. Despite observations which show that the dominant condensed phases on the surface of Mars are solid carbon dioxide and water ice, clathrates have been repeatedly proposed to play an important role in the distribution and total inventory of the planet’s volatiles. Here we review the potential consequences of the presence of clathrates on Mars. We investigate how clathrates could be a potential source for the claimed existence of atmospheric methane. In this context, plausible clathrate formation processes, either in the close subsurface or at the base of the cryosphere, are reviewed. Mechanisms that would allow for methane release into the atmosphere from an existing clathrate layer are addressed as well. We also discuss the proposed relationship between clathrate formation/dissociation cycles and how potential seasonal variations influence the atmospheric abundances of argon, krypton and xenon. Moreover, we examine several Martian geomorphologic features that could have been generated by the dissociation of extended subsurface clathrate layers. Finally we investigate the future in situ measurements, as well as the theoretical and experimental improvements that will be needed to better understand the influence of clathrates on the evolution of Mars and its atmosphere.     

气动计算软件集成系统中的远程控制

随着我国航空航天技术的飞速发展,气动计算软件集成技术日趋成熟,但用户在并行计算中需要手动输入的操作较多。鉴于此,通过编程开发了基于TCP／IP协议的FTP客户端应用程序,实现了对网格文件的信息采集、过滤并将其和参数、脚本文件等批量自动上传的功能。根据批处理文件中的命令,调用Windows平台自带的客户端Telnet,向远程集群管理节点发出命令,远程启动服务器集群的并行计算任务。最后,在客户端实现了远程控制服务器集群上的计算流体力学软件Fluent进行并行计算。结果表明：使用该远程控制系统能够减少用户输入操作,提高计算效率,保证数据的实时更新。