Critical phenomenon,crisis and transition to spatiotemporal chaos in plasmas

In a driven/damped drift-wave system a steady wave induces nonlinear variation of the dispersion of a perturbation wave (PW). Competition between the nonlinear dispersion with self-nonlinearity of the PW results in rich wave dynamic behaviors. In particular, a steady wave at the negative tangency slope of a hysteresis becomes unstable due to a saddle instability. It is found that such saddle steady wave (SSW) plays an important role in the discontinuous transition from a spatially coherent state to spatiotemporal chaos (STC). The transition is caused by a crisis due to a collision of the PW attactor to an unstable orbit of the SSW. In the time evolution, it is a ‘pattern resonance’ of the realized wave with the virtual SSW that triggers the crisis. The transition also displays as a critical phenomenon in parameter space, which is related to the change in the symmetry property of the motion of master mode (k = 1) of the PW with respect to that of SSW. In the spatially coherent state the former is trapped by the SSW partial wave, while in the STC it can become free from the latter, its trajectory crosses two unstable orbits of the SSW frequently, causing very turbulent behavior. This revised version was published online in August 2006 with corrections to the Cover Date.     

坡面浅层明流流态界定方法之商榷

为了探求坡面薄层水流流态界定方法,从流体力学与泥沙运动学观点出发,对4种不同粗糙尺度床面（光滑玻璃、人工加糙粒径分别为0．075、0．245和0．380mm）、5种不同坡度下坡面薄层水流放水进行试验研究,并对薄层水流阻力规律与明渠水流阻力规律进行了比较分析。在此基础上提出了粘性底层厚度与水深之比作为新的无量纲临界判数,结果表明该判数能更好地反映坡面薄层水流流动型态。     

复杂作业模式下车间生产调度的建模与优化

针对某航天制造企业的实际生产环境,分析和讨论了复杂作业模式下车间生产的调度问题,并根据实际的业务流程建立了数学模型,通过自动调度与人工调度相结合的方法对其进行优化,最后采用实例对调度结果进行了验证.事实证明,这种调度机制可以同时增强系统的灵活性和稳定性,对提高车间生产效率和管理水平有很大帮助.     

Solar Radio Bursts with Drifting Stripes in Emission and Absorption

This review covers fairly comprehensively experimental and theoretical research on the fine structure of types zebra pattern (ZP) and fiber bursts (FB) in solar type II + IV radio bursts. The basic attention is given to the latest experimental data. A comparative analysis of several recent solar type IV radio outbursts with these fine structure in dynamical radio spectra is carried out using available ground-based and satellite data (Yohkoh, SOHO, TRACE, RHESSI). New data on microwave zebra structures and fiber bursts testifies that they are analogous to similar structures observed at meter wavelengths. The discovery of the superfine structure, in the form of millisecond spikes is the most significant new effect in the cm range. All basic theoretical models of the zebra pattern and fiber bursts are discussed critically. Two main models are studied for their interpretation: (i) interactions between electrostatic plasma waves and whistlers, (ii) radio emission at double plasma resonance (DPR). The relative significance of several possible mechanisms remains uncertain.     

计算板坯连铸结晶器速度场时计算方程的处理

对计算板坯连铸结晶器内三维速度场时常用的连续性方程的处理方法进行讨论，用有限差分法评述了处理此方程的新途径。     

浅议我国个人所得税实施中存在的问题及解决对策

个人所得税在调节个人收入、增加财政收入、维护国家权益等方面发挥了积极作用,但是随着我国经济的发展,在实施个人所得税中也逐渐暴露出一些问题。本文针对这些问题,进行了深刻的分析,并提出了解决的对策。     

基于神经网络的仿真输出数据的分布识别

分布识别在仿真输出数据的分析中有着重要的理论和实际价值，但长期以来一直没有很好解决，在研究和改进神经网络的基础上，提出用多层感知机ＢＰ网格进行分布识别，给出了基于ＮＮ的分布识别模型，并进行了实验检验，实验结果表明本方法识别效率高，并具有很高的可靠性，可以辅助分析者作出准确的判断。     

光纤捷联惯组四点减振隔振模式分析研究

光纤陀螺捷联惯组减振设计中,经常采用平面四点减振隔振模式。本文结合减振系统对角振动固有频率的特殊要求,建立减振系统动力学模型,对角线振动固有频率比进行分析,通过改变惯组本体组件的质量分布提高角线振动固有频率比,可为光纤捷联惯组减振设计提供一定的指导。     

A star identification algorithm based on radial and dynamic cyclic features of star pattern

A full-sky star identification algorithm based on radial and dynamic cyclic patterns is presented with the aim of solving the “lost-in-space” problem. The dynamic cyclic pattern match is applied with a maximum cumulate comparison method to identify sensor-catalog pairings in initial match, which substantially eliminates the effects of the star position noise, magnitude noise, and false stars. After initial match pairings of stars are obtained, a chain part extension technique is employed to quickly search for the longest match chain as the final result. Experimental results indicate that the proposed algorithm is highly robust to star position noise, magnitude noise and false stars. In a series of simulations, the identification rate of the algorithm is 97.50% with 2.0 pixels star position noise, 96.90% with 0.4 Mv star magnitude noise and 95.30% with four false stars respectively. Moreover, the algorithm achieves an identification rate of 58.08% when only six stars are in the field of view.     

Reynolds number effect on compressible cylindrical cavity flow

Presence of a cavity changes the mean and fluctuating pressure distributions inside and near the cavity. For cylindrical cavity flow, the diameter-to-depth ratio is the dominant factor. In this study, flow is naturally developed along a flat plate with two different lengths, resulting in different incoming boundary layer thicknesses ahead of the cavity. The effect of Reynolds number based on incoming boundary layer thickness on characteristics of mean and fluctuating pressure distributions is addressed. Pressure sensitive paint was also used to visualize the mean surface pressure patterns. The effect of Reynolds number on the classification of compressible cylindrical cavity flow and self-sustained oscillating frequency is not significant. An increase in Reynolds number results in a reduction in the value of differential pressure or momentum flux near the rear edge.