基于压缩感知的金属加筋板兰姆波健康监测技术

针对大型复杂板结构安全评价需要,发展了一种基于压缩感知的金属加筋板结构兰姆波健康监测技术。利用压缩感知技术从稀疏阵列得到的少量检测数据中恢复出加筋板结构中兰姆波的频散特性,并提出了一种将余弦相似度和皮尔森相似度相结合的稀疏阵列兰姆波复合成像方法,以实现加筋板结构中大范围缺陷检测和成像。实验结果表明,压缩感知技术可以恢复出金属加筋板中兰姆波的频率-波数关系,提出的兰姆波复合成像方法能够实现金属加筋板中单缺陷和多缺陷的检测及定位。研究工作为复杂板结构损伤检测提供了一种可行的技术方案。     

Ponderomotive Forces in Cosmos

This review is devoted to ponderomotive forces and their importance for the acceleration of charged particles by electromagnetic waves in space plasmas. Ponderomotive forces constitute time-averaged nonlinear forces acting on a media in the presence of oscillating electromagnetic fields. Ponderomotive forces represent a useful analytical tool to describe plasma acceleration. Oscillating electromagnetic fields are also related with dissipative processes, such as heating of particles. Dissipative processes are, however, left outside these discussions. The focus will be entirely on the (conservative) ponderomotive forces acting in space plasmas. The review consists of seven sections. In Section 1, we explain the rational for using the auxiliary ponderomotive forces instead of the fundamental Lorentz force for the study of particle motions in oscillating fields. In Section 2, we present the Abraham, Miller, Lundin–Hultqvist and Barlow ponderomotive forces, and the Bolotovsky–Serov ponderomotive drift. The hydrodynamic, quasi-hydrodynamic, and ‘`test-particle’' approaches are used for the study of ponderomotive wave-particle interaction. The problems of self-consistency and regularization are discussed in Section 3. The model of static balance of forces (Section 4) exemplifies the interplay between thermal, gravitational and ponderomotive forces, but it also introduces a set of useful definitions, dimensionless parameters, etc. We analyze the Alfvén and ion cyclotron waves in static limit with emphasis on the specific distinction between traveling and standing waves. Particular attention has been given to the impact of traveling Alfvén waves on the steady state anabatic wind that blows over the polar regions (Section~5). We demonstrate the existence of a wave-induced cold anabatic wind. We also show that, at a critical point, the ponderomotive acceleration of the wind is a factor of 3 greater than the thermal acceleration. Section 6 demonstrates various manifestations of ponderomotive forces in the Earth's magnetosphere, for instance the ionospheric plasma acceleration and outflow. The polar wind and the auroral density cavities are considered in relation to results from the Freja and Viking satellites. The high-altitude energization and escape of ions is discussed. The ponderomotive anharmonicity of standing Alfvén waves is analyzed from ground based ULF wave measurements. The complexity of the many challenging problems related with plasma processes near the magnetospheric boundaries is discussed in the light of recent Cluster observations. At the end of Section 6, we consider the application of ponderomotive forces to the diversity of phenomena on the Sun, in the interstellar environment, on newborn stars, pulsars and active galaxies. We emphasize the role of forcing of magnetized plasmas in general and ponderomotive forcing in particular, presenting some simple conceivable scenarios for massive outflow and jets from astrophysical objects.     

逆压梯度湍流边界层中的相干结构

利用流动稳定性理论中一般共振三波的概念对4种定常逆压梯度以及两种变逆压梯度湍流边界层的相干结构进行研究.其中2种变逆压梯度分别为压力梯度由小变大和由大变小,变化的终了具有相同的压力梯度.通过计算得出逆压梯度能够激励相干结构的生成和发展,而且逆压梯度越大作用越强.在变压力梯度流动中,压力梯度由大变小的情况对相干结构的激励最强.此外,逆压梯度使相干结构的流向尺度变小,而展向间距基本在100个粘性长度左右,这些变化趋势与实验以及直接数值模拟结果一致.     

现代超临界翼型设计及其风洞试验

开展了现代超临界翼型的设计研究,对现役飞机的压力分布形态进行了分析,针对现役飞机在巡航状态和阻力发散点的压力分布进行对比,提取了现役飞机超临界剖面设计的要点。采用类函数/型函数变换(CST)参数化方法、基于二阶震荡及自然选择的随机权重混合粒子群算法(RwSecSelPSO)、雷诺平均Navier-Stokes(RANS)方程、Kriging代理模型结合定期望值型的目标函数建立了优化设计系统。针对提高阻力发散马赫数和降低巡航低头力矩的设计指标,利用优化设计系统通过调整目标期望值设计了一系列满足设计指标但阻力发散马赫数不同的超临界翼型,并选择了其中具有典型特性的翼型进行了对比分析,验证了提高阻力发散马赫数和低速失速特性的设计方法,指出了在阻力发散点形成平顶形压力分布的超临界翼型具有较好的综合性能。对设计的超临界翼型进行了高、低速风洞试验验证,试验结果表明:设计结果达到了设计指标要求,提出的低速改进方案有效,层流对超临界翼型失速特性影响较大。     

超声电喷推进微细驻波形成及影响因素分析

对超声电喷推进微细驻波进行了研究,试验观测了微细驻波形成形态,并在不同频率下对比分析了微细驻波波长的理论值和试验值;同时分析了不同推进剂条件下,振动频率对微细驻波波长和形成驻波所需振幅的影响规律。结果表明：不同频率下,形成微细驻波波长的理论值和试验值具有较好的一致性;微细驻波的波长和振幅随着振动频率的增大而减小,同时推进剂的粘度越大,形成微细驻波所需的振幅也越大。     

准平行无碰撞激波的混合模拟

本文应用一维混合模拟方法数值研究了准平行无碰撞激波的结构.结果表明,激波上游的质子和准平行无碰撞激波相互作用后,有部分质子被激波反射,并向激波上游运动很长一段距离,从而激发起束流不稳定性,引起大振幅的共振右旋偏振的低频波动.这些波动在太阳风的带动下向激波下游运动,靠近激波后与激波合井,同时在激波的上游不断有新的波动产生.此过程能不断重复地进行.在平行无碰撞激波的情况下,在激波的下游还有大振幅的非共振右旋偏振的低频波动.激波上游的低频波动在向下游运动的过程中强度不断加强,最后超过原来激波的强度,形成新的激波.      

平流层冬季增温及大气中的行星波

本文利用NIMBUS-7SAMS资料分析了东经100度子午线上的两个站点(67.5°N和42.5°N)在10mb和0.0827mb高度上从1978年底至1982年间的大气温度,获得几年的平流层冬季增温结果.在1978/1979年和1981年初的冬季,高纬站点几天内出现的平流层增温最大幅度可达65K.对平流层增温的谱分析结果指出,在高纬冬季平流层有很强的16天、32夭、21天周期的行星波。中纬冬季平流层增温幅度较小,约为20K.中纬的中间层高度上整年存在有5天、8天和16天的行星波。分析研究、南、北半球不同纬度的温度随经度的分布,得出高纬冬季平流层、中间层大气温度随经度有明显的变化。波数1和波数2的波有大的幅度(主要是波数1),从高纬到低纬,波幅逐渐减小在冬季的平流层和中间层大气中,波数1和波数2的行星波在短期内可强烈增强,引起平流层冬季增温。     

Stochastic acceleration of charged particle in nonlinear wave field

Possibility of stochastic acceleration of charged particle by nonlinear waves is investigated. Spatially regular (SR) and spatiotemporal chaotic (STC) wave solutions evolving from saddle steady wave are tested as the fields. In the non-steady SR field the particle is finally trapped by the wave and averagely gains its group velocity, while in the STC field the particle motion displays trapped-free phases with its averaged velocity larger or smaller than the group velocity depending on the charge sign. A simplified model is established to investigate the acceleration mechanism. By analogy with motor protein, it is found that the virtual pattern of saddle steady wave plays a role of asymmetric potential, which and the nonlinear varying perturbation wave are the two sufficient ingredients for the acceleration in our case. This revised version was published online in August 2006 with corrections to the Cover Date.     

基于声阻抗匹配理论的弹性吸收体研究

基于时域耦合模型理论的吸收体研究,不适用于所有模型,且基于此理论的设计过程复杂,难以在工业工程得到广泛应用。因此提出一种基于声阻抗匹配理论的弹性吸收体的研究方法,并通过理论计算、数值仿真以及实验对吸收体的吸收曲线进行验证。结果表明：本文提出的方法能够快速、简便地实现弹性吸收体的结构设计,无需额外附加阻尼材料,更有利于满足航空工程中对于结构轻量化的要求,同时,为振动波吸收领域,尤其是弯曲波的高效吸收和减振设计研究带来了新的可能性。     

缝隙漏波波导天线及其RCS

介绍了非谐振缝隙组成的漏波波导行波天线，它是在短形波导宽面切铣间距密集的横向短槽构成的线阵；以该线阵为单元设计并研究了驻波平面阵列及其后向ＲＣＳ；给出Ｋｕ波段的天线例子，实验测试结果表明，本天线具有良好的辐射方向图、增益、输入驻波比（ＶＳＷＲ）、带宽和ＲＣＳ特性。