基于OpenGL的快速成形软件开发技术

简要介绍了快速成形软件开发中OpenGL环境的建立方法,分析了软件编写过程中的分层算法有向加权图数据结构和扫描路径的生成算法并给出了应用实例。     

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.     

等厚度楔形杆的应力分析

本文将应力场分为基本应力场和修正应力场两个部分。基本应力场的应力σ_x用勒让德级数展开,级数的前两项系数用截面法确定;其他应力τ_(xy),σ_y由平衡方程和侧表面边界条件确定;再用余能原理确定其余各项系数。由于该级数收敛很快,故可得到封闭解并能给出该解的应用范围,为精确满足自由端的静力边界条件,又引入一个从自由端到固定端迅速衰减的修正应力场,该应力场的应力在自由端等于已知外力与基本应力解之差。其确定方法与基本应力场相同,它也有一个封闭解。将以上两应力场相加卽可得到满足全部边界条件的解。     

一般硬化材料弹塑性旋转盘的变分解法

首先在小弹塑性范围内用应变的奇次四项式相当精确地拟合一般硬化材料的拉伸曲线;再在体积不变条件下用弹性位移场的已知模态和一待定幅值构成弹塑性位移场;最后用势能原理确定该幅值而得到封闭解。     

舰舰导弹武器系统综合作战效能多因素模糊评估

讨论了目前舰舰导弹武器系统作战效能评估中的几点不足,提出了用多因素模糊评估的方法评估舰舰导弹武器系统的综合作战效能。首先,给出了多因素模糊评估模型,包括确定评估因素指标集和加权相对偏差距离最小法的评估步骤;其次,通过对具有典型意义的5种舰舰导弹武器系统的综合作战效能进行多因素模糊评估,给出了应用示例,并对评估模型进行了分析,得出结论。     

线性有源网络拓扑分析的k-连接组法

本文提出了Coates图k-连接组的概念,建立了求解线性有源网络不定导纳矩阵一般k阶余因式的k-连接组拓扑公式,得到了线性有源网络拓扑分析的一种新方法——k-连接组法。与正(负)根有向树法相比,这种方法需找的子图和结果中的冗余项都比较少。     

应力极值分布、强度威布尔分布的可靠性

本文运用应力—强度干涉理论,推导了应力为Ⅰ型极小值分布,强度为威布尔分布的可靠度计算公式,并对冗长的计算公式进行简化,在简化公式的基础上,运用一定的数学技巧,改变积分公式中的积分变量和上下限。将被积函数化成在某一区域内的可积函数。采用de Boor编制的一种严谨的自适应Romberg外推格式的FORTRAN程序进行数值积分。对应予不同的组合参数,给出应力服从Ⅰ型极小值分布,强度服从威布尔分布的可靠度数值。本文最后讨论了服从这两种分布的组合参数的变化对可算度数值变化的影响。     

形态图计算中的投影空间维数和投影空间模型

确定投影空间维数和建立投影空间模型是计算机视觉领域中形态图计算时一个十分重要的基本问题，本文根据态图计算时特征视图拓扑结构等价的特点，指出轴测投影下的投影空间是二维空间，透视投影空间为三维空间，并分别了投影空间模型的建立方法，从而使复杂物体形科计算是简单可行。     

电子干扰对低可观测飞行器飞行路径规划的影响

为了提高巡航导弹的低空突防能力,在分析电子干扰对雷达网威胁区域的影响后认为:在多重干扰条件下,雷达探测空间会顺着干扰方向产生内凹和偏移,因此,建立了新的雷达探测空间模型.采用空间对象间拓扑关系推理方法建立了飞行器飞行路径规划目标函数中雷达威胁指数模型,然后改进了飞行器飞行路径规划模型,并在此基础上进行了巡航导弹飞行路径规划的软件仿真.仿真结果表明:考虑电子干扰对雷达威胁区域的影响情况下规划的飞行路径能够回避雷达威胁,有效提高飞行器低空突防能力.     

耐久性/损伤容限设计简介

概述了飞机结构耐久性／损伤容限设计的基本思想、设计规范及耐久性／损伤容限设计基本理论及方法，供设计人员参考。