关联大系统的中性化分散控制与稳定性

本文提出了一种新的关联大系统中性化分散控制方法,可以使大系统处于非中性关联时的性能等同于子系统全解耦时的性能,确保各子系统有完全的自主性,避免了大系统的参数阵出现摄动,从而改进了关联大系统的整体性能。文中根据向量李亚普诺夫函数,在解耦分散控制子系统渐近稳定的条件下,提出了一种根据中性化关联矩阵判断关联大系统稳定性的方法。     

智能结构有限元模型的建立及静态形状控制

本文建立了含有分布压电传感元件和执行元件的板结构的有限元模型，提出了一种新的具有电自由度板弯曲单元，用于分析含有分布传感元件和执行元件的板结构。以此为基础，提出了智能结构静态形状控制的一般方法，即被动控制方法和主动控制方法。最后，提供了两个数值示例，说明本文提出的方法的应用。     

基于模糊神经网络的涡结构识别方法研究

研究气动光学传输效应产生的机理是红外成像末制导的共性基础技术之一,基于涡结构对光学传输效应进行建模是一种非常有效的方法,而涡结构的识别是其必要前提。文中提出一种新的涡结构识别方法,把折射率场经小波变换后的系数矩阵等效为具有一定纹理结构的图像,计算图像的共生矩阵及其统计量,由于涡结构模式复杂,特征量较多,设计了等价结构的模糊神经网络进行涡结构识别。与小波分解后直接提取特征量的识别方法相比,本文的方法从空、频角度更加准确全面地表征湍流涡结构模式,计算机仿真结果表明该方法优于神经网络的识别效率。     

基于压电智能结构飞机座舱振动噪声主动控制研究

针对在某些特殊情况下飞机座盘舱振动、噪声过大的实际情况，本文对其进行了振动、噪声抑制研究。以某飞机座舱模型为研究对象，利用压电智能结构，并结合振动主动控制方法和LMS自适应滤波算法，实现了一套完整的飞机座舱模型振动、噪声主动控制系统。最后本文给出实验结果，证明了此方法对飞机座舱模型振动、噪声抑制的有效性。     

结构随机跳变系统的条件滤波新方法

提出了不完全状态及控制信息的结构随机跳变系统的滤波方法，解决了结构随机跳变系统在控制入与状态的观测互为相关情况下，系统的状态以及不确知的控制输入的最优估计问题。并以线性高斯情况为例进行了数字仿真，证明了该方法的有效性。     

一种分析气体螺旋槽径向轴承的新方法

论述了一种用非正交坐标系中的流场控制方程分析求解气体螺旋槽径向轴承的新方法,这一方法使得螺旋槽径向轴承的计算和普通滑动轴承的计算一样准确方便。文中还用这种方法计算分析了气体螺旋槽径向轴承的静态性能,获得了一些有益的结论。     

基于MPI的大规模变量结构优化技术研究

针对大规模变量结构优化问题,研究了基于虚载荷法的位移敏度求解理论,提出了惩罚函数随优化迭代次数自适应变化的二次扩展内罚函数法,并结合牛顿法作为优化算法.采用MPI并行技术实现了敏度求解的局部并行计算,解决了大规模变量结构优化技术中的规模和效率问题.采用FORTRAN语言在HAJIF2013系统上对上述方法编程实现,实例表明,优化方法能够快速、稳定收敛到最优解,以及基于虚载荷法的位移敏度解析求解理论的高效性和准确性.     

Cylindrical and spherical dust-electron-acoustic shock waves due to dust charge fluctuation

Cylindrical and spherical dust-electron-acoustic (DEA) shock waves propagating in a dusty plasma (containing cold inertial electrons, hot Maxwellian electrons, stationary and streaming ions, and charge fluctuating stationary dust) are theoretically investigated by reductive perturbation method. It is shown that the effect of the dust charge fluctuation introduces some new features in the nonlinear propagation of the DEA waves, particularly the dust charge fluctuation provides a source of dissipation, and is responsible for the formation of the DEA shock structures. It is also found that the basic features of the DEA nonlinear structures are significantly modified by the non-planar (viz. cylindrical and spherical) geometry, and that the height of the cylindrical DEA shock structures are larger than that of the planar DEA shock structures, but smaller than that of the spherical ones. The implications of these results in laboratory dusty plasmas are briefly discussed.     

Tearing,coalescence and fragmentation processes in solar flare current sheet and drifting pulsating structures

The paper presents a summary of results from two different simulations which study the tearing, coalescence and fragmentation of current sheets, the associated production of energetic electrons and of plasma waves from these electrons which could explain drifting pulsation structures observed at radio wavelengths. Using a 2.5-D particle-in-cell (PIC) model of the current sheet it is shown that due to the tearing mode instability the current sheet tears into plasmoids and these plasmoids later on coalesce into larger ones. During these processes electrons are accelerated and they produce observable electromagnetic waves. Furthermore, the 3-D PIC model with two current sheets extended in the electric current direction shows their fast fragmentation associated with the exponential dissipation of the free magnetic field energy. An example of the drifting pulsating structure which is considered to be a radio signature of the above mentioned processes in solar flares is shown.     

Shear flow energy redistribution stipulated by the internal-gravity wavy structures in the dissipative ionosphere

The linear mechanism of generation, intensification and further nonlinear dynamics of internal gravity waves (IGW) in stably stratified dissipative ionosphere with non-uniform zonal wind (shear flow) is studied. In case of the shear flows the operators of linear problem are non-selfadjoint, and the corresponding Eigen functions – nonorthogonal. Thus, canonical – modal approach is of less use studying such motions. Non-modal mathematical analysis becomes more adequate for such problems. On the basis of non-modal approach, the equations of dynamics and the energy transfer of IGW disturbances in the ionosphere with a shear flow is obtained. Exact analytical solutions of the linear as well as the nonlinear dynamic equations of the problem are built. The increment of shear instability of IGW is defined. It is revealed that the transient amplification of IGW disturbances due time does not flow exponentially, but in algebraic – power law manner. The effectiveness of the linear amplification mechanism of IGW at interaction with non-uniform zonal wind is analyzed. It is shown that at initial linear stage of evolution IGW effectively temporarily draws energy from the shear flow significantly increasing (by an order of magnitude) own amplitude and energy. With amplitude growth the nonlinear mechanism turns on and the process ends with self-organization of nonlinear solitary, strongly localized IGW vortex structures (the monopole vortex, the transverse vortex chain or the longitudinal vortex street). Accumulation of these vortices in the ionospheric medium can create the strongly turbulent state.