预测悬停旋翼跨音速流动的一种组合自由尾流/CFD方法

一种新的组合自由尾流 / CFD方法用于悬停旋翼流动的 CFD解中以考虑实际尾流的作用 .用文中描述的尾流分析方法研究了螺旋尖涡的运动 .首先从广义尾流模型开始 ,用半经验公式模化了涡核对旋翼尾流的作用 ;然后在环量收敛和尾迹收敛的条件下完成了自由尾迹计算 ;最后应用 Jameson有限体积龙格 -库塔推进格式求解了欧拉方程 .所得结果与相关文献和实验数据进行了比较     

战术导弹折叠翼快速展开性能的测试技术

介绍某些战术导弹折叠翼快速展开特性测试技术。详细地介绍了测量方法、项目、数据处理和主要结果。试验是在北京空气动力研究所一座低速风洞中进行的。试验结果表明，获得的数据具有很高精度和可靠性，重复性也是令人满意的。     

在二元柔壁自适应风洞中利用面元法进行三元模型实验

简要叙述了在西北工业大学二元柔壁自适应风洞中利用面元法进行二元半机翼模型试验的研究情况，分析了面元法的基本思想和部分试验结果。     

Solar and Heliospheric Modulation of Galactic Cosmic Rays

The significance of external influences on the environment of Earth and its atmosphere has become evident during recent years. Especially, on time scales of several hundred years, the cosmogenic isotope concentration during the Wolf-, Spoerer-, Maunder- and Dalton-Minimum indicates an increased cosmic ray flux. Because these grand minima of solar activity coincide with cold periods, a correlation of the Earth climate with the cosmic ray intensities is plausible. Any quantitative study of the effects of energetic particles on the atmosphere and environment of the Earth must address their transport to Earth and their interactions with the Earth’s atmosphere including their filtering by the terrestrial magnetosphere. The first problem is one of the fundamental problems in modern cosmic ray astrophysics, and corresponding studies began in the 1960s based on Parker’s cosmic ray modulation theory taking into account diffusion, convection, adiabatic deceleration, and (later) the drift of energetic particles in the global heliospheric magnetic field. It is well established that all of these processes determining the modulation of cosmic rays are depending on parameters that are varying with the solar magnetic cycle. Therefore, the galactic cosmic ray intensities close to Earth is the result of a complex modulation of the interstellar galactic spectrum within the heliosphere. The modern view of this cosmic ray modulation is summarized in our contribution.     

Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton

We present an analysis of seven clusters observed by XMM-Newton as part of our survey of 17 most X-ray luminous clusters of galaxies at z  0.2 selected for a comprehensive and unbiased study of the mass distribution in massive clusters. Using the public software FTOOLS and XMMSAS we have set up an automated pipeline to reduce the EPIC MOS and pn spectro-imaging data, optimized for extended sources analysis. We also developped a code to perform intensive spectral and imaging analysis particularly focussing on proper background estimate and removal. XMM-Newton deep spectro-imaging of these clusters allowed us to fit a standard β-model to their gas emission profiles as well as a standard MEKAL emission model to their extracted spectra, and test their inferred characteristics against already calibrated relations.     

复合材料层板中就位横向拉伸强度的研究

本文利用弹性力学和断裂力学方法对纤维增强复合材料的横向拉伸强度进行了分析，其中考虑了９０度开裂层厚度和开裂邻层的约束效应的影响，推导出正交各向异性对称铺层中昨合就位横向拉伸强度的数学表达式，得出开裂层的厚度和约束邻层铺设角对就位横向拉伸强度都有影响的结论，理论计算与Ｆｌａｇｇｓ实验结果吻合较好。     

关于危险品运输的紧急救援

危险品运输是技术要求最高的一类特种货物运输。在运输、装卸及贮存保管过程中,稍有不慎便会发生事故,造成人身伤亡和财产毁损。笔者认为:灾害=事故十损失。严格执行危险品运输规章,减少事故发生率,从技术上进行要求。仅是问题的一个方面。而另一方面还应立足于事故发生后的紧急救援,以最大限度地减少损失,两者并重才不致酿成灾害。为此,提出了建立“危险品运输紧急救援中心”的建议。     

离心铸造Al—20wt%Si合金自生表面复合材料的组织与性能

采用热模金属型离心铸造Al－20wt％Si合金，获得了外层聚集粗大初晶Si、中层为共晶组织、内层聚集细小初晶Si的自生三层表面复合材料。考察了复合材料的组织形貌，检测了复合材料的硬度和耐性，分析了复合材料的断裂模式。     

0.1米低温风洞的设计

本文阐述了我国首次设计和建造的低温风洞的设计特点及共性能。这是一座以风扇驱动的闭口回流式风洞,用氮气作试验气体。试验段为0.1米的方形截面。计运转参数范围为:M=0.04～0.40,P_t=101.2 kPa～202.6kPa,T_t=79K～320K。试验时间为半小时。风洞壳体是用铝合金制造的,外部用超细玻璃棉绝热。风扇用交流电机拖动,转速用变频控制。     

H-6部件与外挂天平的研制

介绍了H 6部件与外扌圭物测力试验的难点 :一是天平的设计载荷极不匹配 ,如机翼天平的滚转力矩是常规天平的 1 0多倍 ;二是模型尾部是船形尾段。采用常规的支撑方式 ,支杆强度太弱 ,试验不安全 ,同时也不利于多台天平的敷线 ,总体方案采用模型尾部与支杆合为一体的结构形式 ,既保证了试验安全又便于多台天平的敷线。天平设计首先保证试验安全 ,用双电桥提高天平的输出。试验结果表明 :总体试验方案正确 ,天平设计合理 ,支撑刚度好 ,测量精度高。