喷管流场和羽流场的N－S数值模拟

利用时间推进的方法，通过求解可压缩的、雷诺平均的Ｎ－Ｓ方程，并利用Ｂａｌｄｗｉｎ－Ｌｏｍａｘ两层代数滴流模型和Ｐｒａｎｄｔｌ混合长度模型，数值模拟了飞机和火箭发动机喷管的内流和羽流，获得了喷管内流场和羽流场的参数分布，计算结果与试验结果及国外研究成果一致。网格划分采和了自适应网格技术。     

D/H and Nearby Interstellar Cloud Structures

Analysis of UV spectra obtained with the HST, FUSE and other satellites provides a new understanding of the deuterium abundance in the local region of the galactic disk. The wide range of gas-phase D/H measurements obtained outside of the Local Bubble can now be explained as due to different amounts of deuterium depletion on carbonaceous grains. The total D/H ratio including deuterium in the gas and dust phases is at least 23 parts per million of hydrogen, which is providing a challenge to models of galactic chemical evolution. Analysis of HST and ground-based spectra of many lines of sight to stars within the Local Bubble have identified interstellar velocity components that are consistent with more than 15 velocity vectors. We have identified the structures of 15 nearby warm interstellar clouds on the basis of these velocity vectors and common temperatures and depletions. We estimate the distances and masses of these clouds and compare their locations with cold interstellar clouds.     

耐高温有机硅树脂的合成及其耐热和固化性能研究

以甲基和苯基氯硅烷为单体,采用水解缩聚的方法合成有机硅树脂,并对影响有机硅树脂合成的有关因素进行了研究。结果表明,当水解温度为70℃,控制水用量n(H2O)／n(c1)在8:1-5:1的范围内时,可合成出易溶于甲苯的有机硅树脂。红外光谱(IR)显示,合成的硅树脂含有端羟基。采用热失重法(TG)、热失重的微分曲线法(DTG)和马弗炉烧蚀试验研究有机硅树脂耐的热性能和室温固化性能,并对KH-CL和三乙醇胺两种室温固化剂对硅树脂的耐热性能的影响进行了对比研究。结果表明,在氩气气氛下,硅树脂具有很高的耐热性能,它的起始分解温度为400℃,热失重主要由400-500℃时"解扣式"降解和500℃之后的"重排"降解引起。但在空气气氛下,由于有机基团的氧化分解,硅树脂的耐热性有所下降。KH-CL可使硅树脂在室温条件下固化,固化后硅树脂的耐热性能提高。     

微机测控系统输入输出接口智能故障诊断

介绍了用于对微机测控系统输入接口板、输出接口板测试硬件系统的构成,设计了接口卡电路.针对两块电路板,提出了对数字电路板的测试和故障诊断分四个层次,即整板级、功能模块级、单片级和功能输出点级的思想,采取了对功能输出点进行编码的方法建立数字电路板测试的标准知识库,提出了使用功能标志矩阵的方法对各个层次的测试结果进行存储的方法,并根据各个层次测试的关系及相应功能标志矩阵的关系建立了智能化故障诊断程序.     

含孔边裂纹板的弯曲断裂计算

 采用复变函数理论和边界配置方法 ,对含孔边裂纹板的弯曲断裂进行了分析计算。首先假设挠度的复变函数式 ,进而可以求板的内力。它们能满足一系列的基本方程和支配条件 ,仅板的边界条件需要考虑 ,并且可用边界配置法和最小二乘法近似满足。对孔双边裂纹问题进行了应力强度因子计算。数值算例表明 ,本文方法精度较高 ,计算量小 ,是一种有效的半解析、半数值计算方法。     

A lightning swept stroke model: A valuable tool to investigate the lightning strike to aircraft

In the context of lightning strike on the Dassault Falcon family of aircraft, the standard zoning of Falcon 50, 900 and 2000, inferred from FAA and EUROCAE WG31 documents [US Department of Transportation, Federal Aviation Administration, Advisory Circular AC 20-53A, 1985; US Department of Transportation, Federal Aviation Administration, Advisory Circular AC 20-53B, Draft, 1991; EUROCAE WG 31, Aircraft Lightning Zoning Standard, ED-91, 1998], has been presented. Zoning proves to be quite similar between the three types of aircraft. Thanks to the feed-back on lightning strikes to Falcon, lightning traces have been observed on the fuselage for different flight conditions and aircraft. Observations are compared with the zoning performed by Dassault. A physical model, developed by ONERA, was used to simulate the sweeping of lightning on the fuselage of a Falcon 900. The results are in good agreement with the lightning traces observed on the fuselages.     

构建高职数控技术应用专业课程体系的改革与实践

课程体系是衡量学校办学水平和教学质量的重要标志，是实现培养目标的基本保证。从构建课程体系前提、人才培养目标、人才培养机制、课程体系构建、课程体系改革的效果等几个方面对数控技术应用专业课程体系建设进行了探讨，初步构建了产学研结合的人才培养途径，建立了理论体系和实践体系相结合的课程体系。     

Modeling of dynamic evolution of coronal loops

Parameters of expanding magnetic loops and arches and of mass flows generated by them in the corona have been computed in a 1D two-fluid approximation. Two possible trigger mechanisms of the coronal transients have been considered: (i) sudden increase of the background magnetic field strength, and (ii) heating and compression plasma inside these magnetic structures. We discuss the formation of shock waves and their dependence on dynamics and geometry of the magnetic structures.     

图式理论在大学英语阅读中的重要性

本文介绍了图式理论在阅读理解中的作用。实践表明，图式或背景知识在阅读理解中起着极大的作用。因此，在英语阅读中，教师应该把扩展学生的背景知识放在首位，从而可调动学生的阅读积极性，最终提高学生的阅读理解能力。     

Solar Gamma-Ray Spectroscopy

Interactions of ions accelerated in solar flares produce gamma-ray lines and continuum and neutrons. These emissions contain a rich set of observables that provides information about both the accelerated ions and the environment where the ions are transported and interact. Ion interactions with the various nuclei present in the ambient medium produce gamma-ray lines at unique energies. How abundance information is extracted from the measurements is discussed and results from analyses of a number of solar flares are presented. The analyses indicate that the composition of the ambient gas where the ions interact (typically at chromospheric densities) is different from that of the photosphere and more like the composition of the corona, exhibiting low-FIP elemental enhancements that may vary from flare to flare. Evidence for increased Ne/O and the photospheric ³He abundance is also discussed.