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.     

斜爆轰波的波角和法向速度-曲率关系初探

为研究斜劈诱导斜爆轰波的波阵面弯曲效应，以期为斜爆轰的不稳定性及其演化规律提供新的见解，基于加权本质无振荡（WENO）格式空间离散和附加Runge-Kutta方法时间离散的求解器，针对不同的化学反应参数（释热量、放热速率和化学反应区参考长度）条件，开展斜爆轰波的数值计算研究。结果表明斜爆轰波沿波阵面的波角变化可分为3个区域：区域I，波角平滑减小；区域II，波角跃升后衰减；区域III，波角有规律振荡。波阵面法向速度-曲率关系在区域I呈现准垂直直线变化趋势，并伴随着爆轰波强度的不断衰减；在区域III则呈现出"D"形曲线，即由极曲线段、光滑水平变化段和拟线性变化段组成，为类胞格结构的周期性演变；区域II可认为是以上两个区域特征的耦合。不同的化学反应参数对斜爆轰波波阵面的弯曲效应影响存在较大差别。     

Numerical investigation on flow field characteristics of dual synthetic cold/hot jets using POD and DMD methods

In order to improve the control ability of synthetic jets in compressible boundary layer, a novel control method based on dual synthetic cold/hot jets coupled control of velocity profile and temperature profile was proposed. As fundamental investigations on the effects of synthetic jet temperature on the jet behavior and flow field characteristics were essentially necessary, preliminary numerical simulations were conducted to study the influence of temperature (200 K and 400 K) on the flow field characteristics of synthetic jets using Large Eddy Simulations (LES) model. Time-averaged flow fields showed that different temperatures led to variable behavior of two strands of jets. For dual synthetic cold jets, a potential-core arose apparently with its height ranging from 0.01 to 0.03 m, while for dual synthetic hot jets, two strands of jets emerged downstream. The modal decomposition of instantaneous flow fields had been done using both Proper Orthogonal Decomposition (POD) and Dynamic Mode Decomposition (DMD). Various modes showed different characteristics of the flow fields. As the POD method focuses on the energy of flow while the DMD method focuses on the frequency, the first two modes had many similarities, but the third and fourth modes demonstrated completely different vortex structures. The current researches play a role of preliminary investigations for further and comprehensive exploration of novel flow control measures in global velocity field.     

Progress in the Study of Galaxies: Structures,Collective Phenomena and Methods

The review contains the important achievements in dynamics of the galactic disks. Among them there are I. New structures discovered recently: • giant vortices (including giant anticyclone in the Solar vicinity); • slow bar; • inner oscillating structure within spiral arms similar that of enveloped soliton; • chaotic streamlines in the velocity field of the gaseous disk of a real galaxy. II. New collective phenomina discovered recently: • new overreflection instability initiating ‘mini-spiral’ in the innermost central parsec of Galaxy; • large-scale convection caused by nonlinear interaction of density wave with disk gas; • non-kolmogorovian spectrum of weak turbulence corresponding to the observed one in the • Solar vicinity. III. New methods worked out recently: • reconstruction of full three-dimensional vector field of gas velocity from the observed line-of- • sight velocity field; • observational test for verification of the wave-nature of the spiral arms; • observational test to distinguish two types of vertical motions: warp and z-motions in the • density wave; • derivation of correct system of two-dimensional dynamical equations from the initial three- • dimensional one. This revised version was published online in June 2006 with corrections to the Cover Date.     

翼盒结构的可靠性分析及基于系统可靠性的优化设计

 本文研究了翼盒结构的可靠性分析及基于系统可靠性的结构优化设计方法。采用发展了的优化准则法枚举系统的主要失效模式,和Feng的高精度法计算系统破坏概率,提出两个迭代公式进行元件尺寸的优化设计。算例结果表明本文方法是中、大型结构系统可靠性分析及优化设计的有效方法。     

直管式科氏质量流量计对脉动流响应的研究

弹性测量管的振动特性决定了科氏质量流量计的测量精度.以直管科氏质量流量计为例,初步分析研究了流体脉动对其测量管振动特性的影响.建立了被测流体脉动时测量管振动的数学模型;采用Galerkin法对模型进行了处理,将模型转化为受外激励和参数激励联合作用的有耦合多自由度振动问题;用多尺度法对其进行了分析,给出了脉动流作用下科氏质量流量计测量管振动的主要频率成分,揭示了脉动流作用的机理.所得到的大部分结论与有关文献的实验结果吻合.     

基于Lorentz信息度量的分窗二值方法

光照不均是对数字图象进行二值化处理时需要解决的一个问题。在利用 Otsu自动阈值选择法进行分窗二值化的同时 ,给出一种基于 Lorentz信息度量的金字塔数据结构判别过程 ,有效地解决了分窗二值化方法 ,克服光照不均时 ,由于分窗大小而使得窗口内仅含背景 (或对象物 )以致影响二值化正确性这一问题。     

飞机结构部件飞行载荷估算方法研究

介绍一种考虑飞机各部件间相互影响（干扰）的气动载荷估算方法。把该方法用于估算全动平尾的飞行载荷,并用它估算了Ｆ－７全动平尾在对称机动情况下的飞行载荷,且与飞行实侧载荷作了比较。结果表明,估算和实测载荷相差１０％左右。这种估算方法,在飞机设计阶段,可用于估算飞机其它部件（机翼、垂尾等）飞行载荷。     

复合材料夹层结构的弯扭稳定性

对复合材料层合板做面板,蜂窝做夹芯的夹层结构在受到弯、扭载荷作用下的稳定性进行了研究。面板采用对称铺层、等高度蜂窝夹芯,利用能量法对临界载荷进行了计算并给出了一些计算曲线。