弹道式再入航天器的烧蚀防热结构设计

介绍弹道式再入航天器烧蚀防热结构设计,文中说明了方案、材料选择、设计和分析计算。最后评价了这种防热结构。     

模糊自组织网络在刀具磨损状态监测中的应用(英文)

应用模糊逻辑和无教师自组织神经网络进行车削过程刀具磨损状态监测.根据典型切削条件组合建立由多个子网络组成的自组织网络阵列,其中每一子网络对应一种典型切削条件,并进行训练.对于具体切削条件,运用模糊逻辑技术选取对应的优化子网络.文中所建名为Fuzzy-SOM-TWC监测系统的运行基于加工过程实时采集的切削力、声发射以及电机电流信号.切削实验用于训练和检验监测系统,实验结果显示其对于刀具磨损状态的识别正确率可达到98%-100%.     

谐波信号的通用频谱校正算法在回转机械监测中的应用

分析了常规FFT谱由于能量泄漏和栅栏效应,不能获得简谐振动信号精确幅值、频率和相位的原因。针对现有校正频谱方法的不足,提出了基于黄金分割的通用频谱校正算法。经仿真实例验证,该方法具有计算量小、校正精度高、适应面广的特性。经过回转机械启动实例分析,该方法能得到准确的临界转速、升速曲线和幅频响应曲线,为回转机械的瞬态行为分析提供了新的手段。     

惩罚函数法在发动机性能计算中的应用

按照涡喷发动机工作时遵守的气动热力学定律，建立了发动机的稳定数学模型，并针对双轴涡轮发动机性能计算的非线性数学模型，利用优化和最优控制理论中的惩罚函数法，对发动机性能进行了基于约束的最优求解程序设计，利用程序对某型发动机的稳定飞行特性进行了计算，计算结果表明，使用惩罚函数法求出的特性曲线变化规律正确，发动机平衡方程的解的精度更高，在此基础上得出的发动机飞行特性也更准确。另外惩罚函数法对初值的要求很低，迭代运算不易发散。     

褶皱结构成形时的形状偏差计算

解决了褶皱结构成形时相邻的平行四边形平面元素之间连接区棱的修圆半径值预测问题。把毛坯模拟成薄板，定义了平行四边形平面元素的边界条件，采用能量法导出挠度和力函数的非线性微分方程组，利用积分－差分法实现其数值解，并提供计算结果和分析应力－应变场。采用的计算方法可用于研究毛坯的刚度参数和工艺参数对褶皱结构的形状影响。     

面内荷载作用下混合型边界约束复合材料层合板的振动特性

本文研究一对边界为混合型约束时矩形层合薄板的振动特性问题。文中同时考虑中面荷载作用效应，给出了基于子域分解技术，单向DQ离散格式和Galerkin法的半解析算法，并通过算例讨论了混合边界构成，铺设方式和面内荷载等对板振动特性的影响。     

二维多介质流动问题的界面处理方法

就二维可压缩多介质流动问题的数值模拟,给出了一种新的界面处理方法。通过在界面处构造Riemann问题,利用Riemann问题的解分别定义界面两边流体的边界条件,由于Riemann问题的解准确地描述了界面处流体的流动状态,因此得到了更加准确的界面边界条件。本文将由Riemann问题的解得到的界面速度外推到整个流场,重新定义速度场,避免了由于速度的大梯度变化而导致的Level—Set等值线相互交错,因而得到了更加精确的界面位置。利用该方法对水下激波与柱型气泡相互作用问题进行数值模拟,结果表明该方法能准确地捕捉各种物理现象。     

Interplanetary shocks and sudden impulses during solar maximum (2000) and solar minimum (1995–1996)

In this work a study is performed on the correlation between fast forward interplanetary shock parameters at 1 Astronomical Unit and sudden impulse (SI) amplitudes in the H-component of the geomagnetic field, for periods of solar activity maximum (year 2000) and minimum (year 1995–1996). Solar wind temperature, density and speed, and total magnetic field, were taken to calculate the static pressures (thermal and magnetic) both in the upstream and downstream sides of the shocks. The variations of the solar wind parameters and pressures were then correlated with SI amplitudes. The solar wind speed variations presented good correlations with sudden impulses, with correlation coefficients larger than 0.70 both in solar maximum and solar minimum, whereas the solar wind density presented very low correlation. The parameter better correlated with SI was the square root dynamic pressure variation, showing a larger correlation during solar maximum (r = 0.82) than during solar minimum (r = 0.77). The correlations of SI with square root thermal and magnetic pressure were smaller than with the dynamic pressure, but they also present a good correlation, with r > 0.70 during both solar maximum and minimum. Multiple linear correlation analysis of SI in terms of the three pressure terms have shown that 78% and 85% of the variance in SI during solar maximum and minimum, respectively, are explained by the three pressure variations. Average sudden impulse amplitude was 25 nT during solar maximum and 21 nT during solar minimum, while average square root dynamic pressure variation is 1.20 and 0.86 nPa^1/2 during solar maximum and minimum, respectively. Thus on average, fast forward interplanetary shocks are 33% stronger during solar maximum than during solar minimum, and the magnetospheric SI response has amplitude 20% higher during solar maximum than during solar minimum. A comparison with theoretical predictions (Tsyganenko’s model corrected by Earth’s induced currents) of the coefficient of sudden impulse change with solar wind dynamic pressure variation showed excellent agreement, with values around 17 nT/nPa^1/2.     

Research on a complex CME event including Hα, LASCO, radio and MDI observations

We present our research on a fast and decelerating partial halo coronal mass ejection (CME) event detected in multi-wavelengths in the chromosphere and the corona on 14 October, 1999. The event involved a whole complex active area which spanned more than 40° of heliolongitude. It included a strong solar flare (XI/1N) and a complex eruptive filament within an active region of the entire complex. Especially, several radio sources were detected in the decimetric range prior to the CME by the Nançay Radioheliograph (NRH). A linear force-free field extrapolation of the Michelson Doppler Imager (MDI) magnetogram was performed to calculate the magnetic topology of the complex prior to the triggering of the event. The presence of a coronal null point combined with the occurrence of two distant and nearly simultaneous radio sources put strong arguments in favor of the generalized breakout model for the triggering of the eruption. The analysis of the subsequent development of the event suggests that large interconnecting loops were ejected together with the CME.     

Pareto最优解的充分及必要条件

对多目标优化问题不需目标函数的凸性和二次可微性的假设，在约束区域具有严格点凸性的条件下，证明了Ｋｕｈｎ－Ｔｕｃｋｅｒ条件是严格局部Ｐａｒｅｔｏ最优解的必要的充分条件，并以若干例子说明其适用性。