航空发动机燃烧室喷油环三维流场数值模拟

针对所研究喷油环的结构特点, 采用四面体非结构化网格和疏密结合的网格划分方法, 生成喷油环网格计算模型, 对喷油环三维流场进行数值模拟计算, 较为详细地分析了单个喷嘴内部流场特性以及喷油环的出口流量分布情况.计算结果为进一步研究喷油环流量分布特性提供了坚实的基础.      

三维五向圆型编织复合材料细观分析及弹性性能预测

 基于三维圆型编织的主要工艺,系统研究了三维五向圆型编织的纱线交织结构,建立了内部单胞和表面单胞模型。推导了单胞的几何特性、编织工艺参数之间的数学关系。基于此模型,采用改进的刚度平均化方法,计算了三维圆型编织复合材料的弹性性能参数,并与实验的结果进行了对比,吻合较好。分析了编织角和纤维体积含量对弹性性能的影响,结果表明,五向圆型编织复合材料保持了四向圆型编织复合材料良好的力学性能,同时由于轴纱的加入,使得轴向的力学性能得以提高。     

Effects of Atomic Oxygen Irradiation on Transparent Conductive Oxide Thin Films

作为一种功能薄膜,透明导电氧化物(TCO)薄膜在飞行器的抗原子氧(AO)涂层和太阳能电池领域有着巨大的应用价值。ZnO:Al(ZAO)和In2O3:Sn(ITO)薄膜是目前研究和应用最广泛的TCO。本文对ITO薄膜和ZAO薄膜进行了不同通量的AO辐照。通过对辐照前后样品的X射线衍射、扫描电镜及霍耳效应的表征及测试,研究了AO辐照对这两种TCO薄膜的结构、性能及电学特性的影响。研究表明AO辐照对ZAO薄膜表面有明显的侵蚀作用,但对其结构和导电性能没有明显影响。对于ITO薄膜,随着AO通量的增大,其载流子浓度逐渐下降从而导致了电阻率的提高,电阻率的最大变化达到了21.7%。     

SHS法反应合成Al3Ti/Al复合材料的研究

通过将5Al-Ti体系混合粉末预制块在一定温度下预热,原位制备出Al3Ti/Al复合材料,并探讨了其生成机理和影响因素.研究发现:Al粉和Ti粉混合预热生成Al3Ti是由Al粉的熔化诱导;在高于热爆起始温度下预热时,Al3Ti直接以热爆反应机制生成;在低于热爆起始温度下预热时,Al3Ti按扩散-热爆反应机制生成.预热温度、Ti粉粒度及冷却速度是影响材料组织性能的关键因素.通过适当工艺制备出具有性能优异的Al3Ti/Al复合材料,其硬度是铝基体的3.6倍,耐磨性高.     

Ion dynamics associated with Alfven wave in the near-Earth magnetotail: Two-dimensional global hybrid simulation

Ion dynamics in the near-Earth magnetotail region is examined during periods of fast Earthward flow with a two-dimensional (2-D) global-scale hybrid simulation. The simulation shows that shear Alfven waves are generated at x ∼ −10R_E, where the strong earthward flow is arrested by the dipole field, and propagate along field lines from the equator to both southern and northern polar ionosphere. Non-gyrotropic ion velocity distributions occur where the large-amplitude Alfven waves are dominant. The simulation indicates that the Alfven waves are generated by interaction of the fast earthward flow with the stationary near-Earth plasma. Beam ions are found to be pitch-angle scattered and trapped in the wave field, leading to the non-gyrotropic ion distributions in the high-latitude plasma sheet boundary. In addition, significant particle heating and acceleration are found to occur behind the dipolarization front due to the effect of wave turbulence.     

嵌入式Linux开发环境建立的方法

文章针对S3C2410x处理器，在宿主机上配置嵌入式Linux系统开发环境。详细叙述了配置的过程、可能出现的问题及其解决方法。     

A 2-D comparison of ionospheric convection derived from SuperDARN and DMSP measurements

Ion drift vectors measured by the DMSP satellites are compared with plasma convection vectors obtained by the SuperDARN HF radars through the standard Map Potential algorithm of Ruohoniemi and Baker [Ruohoniemi, M., Baker, K.B. Large-scale imaging of high-latitude convection with super dual auroral radar network HF radar observations. J. Geophys. Res. 103, 20797–20811, 1998]. Despite significant data spread, the agreement can be qualified as reasonable for a data set comprising of 149 satellite passes over the Northern Hemisphere at high latitudes. The slope of the best-fit line relating SuperDARN and DMSP velocity magnitudes is of the order of 0.3 with a tendency for the SuperDARN velocities to be smaller. The agreement between the azimuths of the ion drift and convection is better with the slope of the best-fit line being close to 1. It is shown that consistency between the radar and satellite measurements is much better if the SuperDARN line-of-sight velocities are compared with the DMSP cross-track ion drifts for events showing slow spatial and temporal variations of the convection. If areas of strong convection changes are included into comparison, the degree of agreement deteriorates drastically. This result implies that differences in the spatial and temporal resolutions of DMSP and SuperDARN measurements are crucial factors contributing to the observed discrepancies. In addition, some differences are introduced when the SuperDARN line-of-sight velocities are filtered and reprocessed into vectors with the application of a background convection model.     

用MultiGen建模与Performer类库实现实时窗外视景

介绍了如何利用MultiGenCreator建造适合Performer高效运行的模型,以及在SGI图形工作站上用Performer实现塔台模拟机的视景系统。重点介绍了如何改进模型使其能在程序中方便的组织和控制,并提出了运动目标的模拟。     

Development of TY-3 Microgravity Rocket System

TY-3微重力火箭总长 6 0 0 0 mm,起飞质量 1 1 0 0 kg,有效载荷 5 0 kg,最大飞行高度 2 2 0 km,能提供 1 0 - 4 g约 36 0 s时间的微重力试验条件 ,该火箭已于 2 0 0 0年 1 0月飞行试验成功 ,而且一种更先进的微重力火箭系统正在设计中。     

连接压力在Ti/Ni/Ti复合层TLP扩散连接Si3N4陶瓷中的作用机制

研究了Ｔｉ／Ｎｉ／Ｔｉ复合层ＴＬＰ扩散连接Ｓｉ３Ｎ４陶瓷时压力对接头形成的作用机制。结果表明,ＴＬＰ来不及与陶瓷发生充分反应并形成高强度结合界面就已完全凝固,为形成高强度的结合界面,必须进一步发生固态扩散反应。只有当连接过程中施加足够的压力,才能保证ＴＬＰ在其存在期间充分铺展陶瓷,并在ＴＬＰ完全凝固后形成大量扩散通道,为固态扩散反应提供必要条件。