含孔边裂纹各向异性有限板的二维问题

应用边界元法,并结合一种特殊的复变函数基本解,研究了含孔边裂纹的各向异性有限板的应力强度因子修正系数的计算。这种特解边界元法避免了在裂纹附近划分单元,可以获得较好的数值计算精度。通过算例分析,结果表明本方法精度高,运算量小,具有一定的工程应用价值。     

飞行器雷达罩设计方法的研究

详细分析了飞行器雷达罩设计过程中的基本问题。基于多目标优化设计方法建立了雷达罩结构参数求解的数学模型,给出了求解方法。考虑到雷达罩的安全使用要求,分析了雷达罩防雷击部件的基本要求,提出了设计方法,给出了防雷击部件布置的经验公式。同时还研究了用于飞行器雷达罩金属部件的吸波材料电磁波吸收机理,以及吸波材料电性能设计原理和基本布置准则     

基于Petri网的空中交通管制辅助决策系统

空中交通管制系统是生产实际中的一种典型的离散事件动态系统（Ｄｉｓｃｒｅｔｅ ｅｖｅｎｔ ｄｙｎａｍｉｃｓｙｓｔｅｍ,ＤＥＤＳ）,而Ｐｅｔｒｉ网理论是研究ＤＥＤＳ的有力工具之一。为了描述空中交通管制系统受到外部控制的交互机制及层次结构,文中引入Ｐｅｔｒｉ网概念的一类扩充－－开放Ｐｅｔｒｉ网的概念,并用开放Ｐｅｔｒｉ网工中交通管制辅助决策系统进行建模与分析,阐述了空中交通管制辅助决策系统的开放Ｐｅｔｒ     

低速高湍流度90°弯管流动数值模拟

分析了曲率对弯曲管道流动的影响 ,给出了曲率修正的双层 k-ε湍流模型 ,并数值模拟了非均匀来流低速高湍流度 90°弯管内流动。文中比较了曲率修正双层 k- ε湍流模型的计算结果与实验结果 ,以及双层 k- ε湍流模型和逆压力梯度修正双层 k- ε湍流模型的计算结果。通过比较 ,发现经过曲率修正后的双层 k- ε湍流模型更好地模拟了非均匀来流低速高湍流度 90°弯管内流动。同时比较了壁面参数的插值方法 ,发现在弯曲管道流动模拟中对壁面参数进行一阶插值比零阶插值能更好地模拟真实流场     

提高电铸局部电沉积速率试验研究

电铸成型是采用离子沉积的方法制造复制件，具有很好的复制精度，因此电铸技术得到了广泛的应用。但由于受极限电流密度等多方面因素的影响，电铸速率一直是制约电铸技术发展的一个瓶颈，许多学者为此做了大量的理论和试验研究，但对如何提高极限电流密度还没有提供一个比较满意的答案，为提高电铸局部电沉积速率，本文在前人工作的基础上，讨论了影响电铸速率的因素，提出了一种新型的电铸方法－喷射式电铸，并通过两组试验分析了局部电沉积速率怀电铸液流量的关系以及局部铸速率与喷嘴口径的关系，试验结果表明，采用喷射式电铸可以大大提高局部极限电流密度，从而使电铸局部电沉积速率有一个较大范围的提高，为将电铸与快速成型结合奠定了试验基础。     

尾流作用下对转涡轮叶片振动的流固耦合数值分析

采用对转涡轮设计可以提高喷气发动机的推重比.本文应用ANSYS/CFX软件,采用流固耦合数值分析方法对低压涡轮转子叶片进行了分析.对一定的涡轮工况,得到了高压涡轮转子叶片尾流作用下的低压涡轮转子叶片振动的应力和变形变化规律.采用傅里叶变换,对流体激励力、叶片应力及变形相应进行频谱分析,结果表明:在复杂来流激励下,叶片的第一阶振动较易被激起;但高阶振动响应不可忽略;而且叶身温度场不同,被激起的振动阶次也不同.     

多孔复合微结构的制备与减反射性能

主要研究了多孔-金字塔和多层多孔-金字塔两种多孔复合微结构的减反射性能。多孔-金字塔是将带有金字塔结构的单晶硅片置于HF/Fe(NO3)3溶液中二次化学腐蚀得到的,而多层多孔-金字塔复合微结构是将带有金字塔结构的单晶硅片置于HF/CH3CH2OH溶液中二次电化学腐蚀得到的。用扫面电镜和UV-vis-NIR分光光度计分别分析了这两种复合结构的表面形貌和反射率。结果表明,在400~800 nm波长范围内,多孔-金字塔和多层多孔-金字塔复合微结构的平均反射率分别为5%和2.1%。多孔-金字塔微结构表面的孔洞较大,表面的金字塔有少量的塌陷,但多层多孔-金字塔微结构表面的孔洞细小且覆盖均匀,表面的金字塔基本上保持完好。通过比较,电化学方法制备的多层多孔-金字塔复合微结构的减反射效果要优于采用化学腐蚀制备的多孔-金字塔复合微结构的减反射效果。     

Dynamics of Planetary Waves in the Ionosphere as Observed from GPS Satellites

The GPS satellite data are used to study the dynamics of the ionospheric total electron content (TEC) over Central Europe in the summer season from June 23 to September 30, 1996. The TEC variations within the range of periods typical of the planetary waves were found to be nearly synchronous with the neutral wind variations in the mesosphere and with the variations in the occurrence of ionospheric sporadic layers. The observed TEC variations were interpreted as the result of penetration of energy carried by nonstationary Rossby waves to the upper atmospheric altitudes.     

A statistical study of C IV regions in 20 Oe-stars

In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of absorption clouds and analyse their characteristics. From this analysis we can calculate the values of a group of physical parameters, such as the apparent rotational and radial velocities, the random velocities of the thermal motions of the ions, the Full Width at Half Maximum (FWHM), the optical depth, as well as the absorbed energy and the column density of the independent regions of matter, which produce the main and the satellite clouds of the studied spectral lines. Finally, we present the relations between these physical parameters and the spectral subtypes of the studied stars and we give our results about the structure of the C IV region in their atmosphere.     

Latitudinal variation of the topside electron temperature at different levels of solar activity

A database of electron temperature (T_e) measurements comprising of most of the available satellite measurements in the topside ionosphere is used for studying the solar activity variations of the electron temperature T_e at different latitudes, altitudes, local times and seasons. The T_e data are grouped into three levels of solar activity (low, medium, high) at four altitude ranges, for day and night, and for equinox and solstices. We find that in general T_e changes with solar activity are small and comparable in magnitude with seasonal changes but much smaller than the changes with altitude, latitude, and from day to night. In all cases, except at low altitude during daytime, T_e increases with increasing solar activity. But this increase is not linear as assumed in most empirical T_e models but requires at least a parabolic approximation. At 550 km during daytime negative as well as positive correlation is found with solar activity. Our global data base allows to quantify the latitude range and seasonal conditions for which these correlations occur. A negative correlation with solar activity is found in the invdip latitude range from 20 to 55 degrees during equinox and from 20 degrees onward during winter. In the low latitude (20 to −20 degrees invdip) F-region there is almost no change with solar activity during solstice and a positive correlation during equinox. A positive correlation is also observed during summer from 30 degrees onward.