蝴蝶翼面形状对绕流结构的影响

蝴蝶的扑翼飞行因其相对翼展较大、扑翼频率低等特点引起广泛关注,尤其是具有越洋迁徙特性的蝴蝶更是备受瞩目。本文以天堂鸟翼凤蝶和黑脉金斑蝶这两种长距离迁徙蝴蝶作为研究原型,利用氢气泡流动显示技术研究这两种不同外形的蝴蝶翼面绕流结构随迎角的变化。在相同的实验条件下,两种模型翼面绕流均出现前缘涡、翼尖涡等流动结构,且绕流结构随迎角的变化趋势基本相同。但由于翼面外形的不同,两种模型在前缘涡的形态、强度及后翼面翼尖绕流结构等方面表现出一定的差异。     

航空维修结构工程师培训的探索与研究

随着民用飞机使用年限和飞行循环的增长，飞机面临的结构问题越来越多。航空公司对于结构工程师的人力需求，对工程师的能力、经验和技术管理的要求也越来越高。山东太古结合自身的维修管理和支援经验，经过数年的探索和实践，建立了较为完善的结构工程师培训体系。     

MDS图在液态模锻工艺过程单片机仿真控制系统中的应用

本文介绍了液态模锻工艺过程单片机仿真控制系统的设计方法，包括液态模锻工艺程确立、逻辑量确立、硬件系统设计、ＭＤＳ图的建立及软件实现，在工艺设备的逻辑性控制中应用ＭＤＳ图控制结构设计的控制器可方便方便地实现ＰＬＣ的控制功能，也可主便地实现其他娄字逻辑系统的控制功能。     

电工实验"MCAI"课件的制作

本文介绍电工实验“MCAI”课件的制作思想和方法。     

Galactic Evolution of the Light Elements: A New Set of B Observations

The boron 2500 spectral region has been observed with the Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope (HST) in a new set of metal-poor stars and analyzed by spectrum synthesis technique, adopting the most recent model atmospheres. By taking into account the Li and Be abundances available from the literature for this same set of objects, the resulting patterns of their light elements abundances cannot be easily justified with the currently known stellar structure scenarios. The finding of real differences in the B content between stars with very similar stellar characteristics suggest that also production effects, rather than depletion and/or mixing only, should be taken into account as a possible and valuable explanation.     

我国税制结构的优化

随着经济的发展和税源结构的变化，税制结构的调整显得十分必要和紧迫，笔者分析了制约我国税制结构优化的因素、税制结构优化的标准，现行税制结构中存在的主要问题，并对优化我国税制结构的措施提出了具体看法。     

钯改性镍基高温合金铝化物涂层的组织和热腐蚀性能

以M38合金作基材，先电镀Pd-20wt%Ni合金，再采用传统低温高活性(LTHA)固渗铝工艺，用NaCl作活性剂渗铝制得Pd-Ni-Al涂层。XRD和EPMA分析结果表明，涂层为固溶Ni的β-PdAl单相结构；在900℃Na     

卫星结构中的非金属材料

介绍了各种复合材料、胶粘剂、高分子材料和工业陶瓷等非金属材料的性能及其在卫星结构中的应用情况。强调了非金属材料在提高卫星性能、减轻卫星结构质量，以及增大卫星有效栽荷方面的作用。最后指出了卫星结构材料高性能、多功能、复合化、智能化、低成本以及高环境相容性的发展趋势。     

Solar Models with Non-Standard Chemical Composition

The OPAL monochromatic opacity tables are used to evaluate the impact of a non-standard chemical composition on solar models. A calibrated solar model with consistent diffusion including the effect of radiative forces and ionization on drift velocities is presented. It is shown that surface abundances are predicted to change slightly more than in traditional solar models where these refinements are not included. All elements included in the model settle at similar rates which is reflected in the relative variation in surface abundances ranging from 7.5% for calcium to 8.8% for argon. The structural difference between the consistent model and the traditional model is small, with a maximum effect of 0.3% for the isothermal sound speed at the base of the convection zone. The settling of CNO is only marginally affected. Opacity profiles have also been calculated with varying abundances for volatile elements, for which the abundances are poorly known, and other selected elements. It is shown that if one allows a 10% variation of these elements individually one can expect a peak Rosseland mean opacity variation of 3% for oxygen, a little less 2% for Si and Ne, and around 1% for Mg and S in the radiative zone. Other light metals and volatile elements have no significant impact on the opacity. This revised version was published online in June 2006 with corrections to the Cover Date.     

圆球绕流场的尾涡分析和升阻力研究

采用自编的分块算法程序模拟了雷诺数在20～1000之间的圆球绕流场.在Re=25时捕捉到流动分离,与试验结果一致.对Re=250时稳态非对称尾流区内流体的输运情况进行研究,证实圆球绕流场中纵向对称面的存在.对于非稳态流动,主要研究了阻力和横向力的时间变化规律,并分析了频谱特征.计算发现横向合力主要在横截面上两个很窄的区间内偏移.经过几种不同涡定义方法的优劣测试,本文采用Hunt等人介绍的Q-定义方法对非稳态绕流场的尾涡结构进行了直观描述.