机载计算机安装架的强度计算

:叙述用有限元计算方法对特定的机载计算机安装架进行结构强度计算 ,内容包括静强度计算、结构自由振动分析和波形为后峰锯齿波的冲击载荷作用下的冲击响应分析。计算结果对安装架的设计具有重要的指导意义。     

On the modular approach of a 3D model of the system magnetosheath–magnetosphere

This article presents some preliminary features of a new self consistent model of the system magnetosheath–magnetosphere, recently developed in the Institute of Mechanics, Sofia, Bulgaria. The flow in the magnetosheath is governed by 3D ideal gas-dynamic equations. The positions and the shapes of the bow shock and the magnetopause are calculated iteratively as a part of the solution. These surfaces are essentially three-dimensional (generally non-axially-symmetric). The self-consistency between the regions is ensured via the boundary conditions. The magnetopause cusp indentations are formed, influencing essentially the magnetosheath flow. Prediction of the position and the shape of the bow shock for different values of the sonic Mach number are derived. Distribution of some flow parameters in the magnetosheath is presented. 3D numerical finite element model, calculating the field due to the magnetopause currents for an arbitrary magnetopause geometry, is used in the magnetosphere. The fields due to the current systems inside the magnetosphere(cross-tail current, ring current, and Birkeland current) are taken from the Tsyganenko empirical model. The magnetopause surface is calculated from the requirement the outside gas-dynamic pressure to be balanced by the magnetic pressure inside. The magnetosphere model can be viewed as an improved version of the empirical model but with more realistic magnetopause form and shielding field. Not a final but a beta version is used in this approach. The final model version as well the model details will be presented elsewhere.     

Anomalous Cosmic Rays and Solar Modulation

We review aspects of anomalous cosmic rays (ACRs) that bear on the solar modulation of energetic particles in the heliosphere. We show that the latitudinal and radial gradients of these particles exhibit a 22-year periodicity in concert with the reversal of the Sun's magnetic field. The power-law index of the low energy portion of the energy spectrum of ACRs at the shock in 1996 appears to be -1.3, suggesting that the strength of the solar wind termination shock at the helioequatorial plane is relatively weak, with s 2.8. The rigidity dependence of the perpendicular interplanetary mean free path in the outer heliosphere for particles with rigidities between 0.2 and 0.7 GV varies approximately as R2, where R is particle rigidity. There is evidence that ACR oxygen is primarily multiply charged above 20 MeV/nuc and primarily singly-charged below 16 MeV/nuc. The location of the termination shock was at 65 AU in 1987 and 85 AU in 1994.     

具有后挡板的喷流流场的数值研究

本文对发射台底面与后挡板之间的喷流流场进行了数值研究。采用迎风的Ｐｅｔｒｏｖ－Ｇａｌｅｒｋｉｎ有限元方法求解欧拉方程。描述了喷流出口处及挡板附近的流场细节。计算结果已成功地应用于导弹发射台的设计。     

喷流流场旋涡激波干扰的数值模拟研究

本文采用隐式CSCM格式,通过数值求解NS方程,对平板上二维超声速主流中横向喷流流场进行了数值模拟,并与实验和其它计算结果进行了分析比较,结果令人满意。     

旋转冲压发动机驻涡燃烧技术研究现状分析

旋转冲压发动机是一种全新概念发动机，采用激波增压和驻涡燃烧技术。其显著的高效、低污染特性引起越来越多人关注。本文首先扼要介绍了旋转冲压发动机总体结构，然后介绍了驻涡燃烧技术的概念和研究现状，最后描述了旋转冲压发动机中驻涡燃烧室的结构特点。     

压缩拐角区的压力,热流工程计算方法

 <正> 引言 从压缩拐角分离流动的试验及数值计算出发,建立起一个实用范围较广精度较高的工程估算程序,方便快速地估算出压缩拐角分离区和再附区的峰值压力、峰值热流;分离区和再附点位置;分离区长度等。这是气动设计部门关注的课题。这些工作是在文献(3,4)中的经验公式的基础上,按照分离流动流谱,分区进行迭代修正计算,对二维情况给出了完整     

再人飞行器脉动压力环境的分析与预测

本文分析了机动再入飞行器因非定常空气动力流动引起的物面脉动压力环境,并根据高超声速无粘流计算的表面压力分布,给出了一套预测各种脉动压力环境统计特性的工程计算公式。算例表明,预测的均方根脉动压力、功率谱密度和交叉功率谱密度与实验值是一致的。     

可压缩球涡和平面激波相互作用的数值研究

行进了可压缩球涡和平面激波相互作用的数值研究。一方面，用非定常Ｅｕｌｅｒ方程数值模拟了一种可压缩球涡的自身演化，同时，利用Ｒａｎｋｉｎｅ－Ｈｕｇｏｎｉｏｔ关系，在流场中嵌入运动激波，求解了激波－球涡相干的流动过程。     

激光干涉技术在振动冲击中的应用

振动冲击计量标准中采用激光干涉仪作为量值溯源工具，本文就振动冲击实验室应用的两类干涉仪从光学原理方面进行一些简单的分析对比。给出了二者之间的一些相同和类似点。