铝/ZN-1阻尼材料复合结构件的粘接技术研究

探讨了胶黏剂黏度、硬铝表面处理方式及硅烷偶联剂KH-560的使用方式等因素对硬铝板/ZN-1阻尼材料复合结构件的粘接性能的影响。研究表明：如果硬铝板表面采用砂纸打磨处理时，采用黏度较低的TC-1环氧树脂胶或者在黏度较高的J-22环氧树脂胶中添加2％的硅烷偶联剂KH-560可以获得优异的粘接效果；当硬铝板表面采用铬酸阳极化处理时，两种胶黏剂均能获得优异的粘接效果。     

叶轮机械三维粘性动静叶干涉的数值模拟

本文发展了 1套模拟叶轮机械三维粘性动静叶干涉的数值方法。在成熟的空间离散方法基础上 ,提出了 1种高效的双时间步隐式时间推进方法 ,并构造了一种保证守恒的动静叶交界面处的数值通量计算方法。本文对某三维亚音速涡轮的动静叶干涉进行了数值模拟 ,结果与实验符合较好。     

测量机连续扫描控制系统设计

利用UCC1控制器作为核心,构建具有三维空间连续扫描功能的测量机控制系统的方法,并简要介绍了UCC1控制器的功能及控制系统硬件电路的设计。     

CVD-Si3N4陶瓷及其复合材料氧化行为研究进展

概述了CVD—Si3N4陶瓷及其复合材料在干燥氧气下的氧化行为。Si3N4陶瓷在高温下氧化时，除生成SiO2保护膜外，还生成一薄层比SiO2膜更优异的氧气扩散阻挡层(Si—O—N化合物层)，该层具有优异的抗氧化性能。介绍了两种氧化机制模型，同时分析了温度、杂质等对CVD—Si3N4陶瓷氧化行为的影响。     

应用ART1神经网络仿真车间分组

阐述了ART1神经网络在制造单元设计过程中形成零件族的基本方法,并在基于MATLAB的软件平台上,利用其神经网络工具箱对生产过程中的实际情况进行了仿真和应用。     

基于Solid Works和Cosmos的模具结构三维设计及有限元分析

复杂结构注塑模具的设计和强度、刚度分析是注塑行业的重要难题。利用Solid Works三维设计软件实现了注塑模具的三维实体建模，并运用COSMOS／Works软件对注塑模具的典型部件进行了有限元分析，验证设计的零件是否符合实际工作情况是实现注塑模具现代化设计的重要途径。通过GearTrax2001Plus、Toolbox等外挂、内挂插件的使用．大大地简化了建模过程，克服了原有设计方法的不足．为解决较复杂的结构设计和理论分析问题提供了一种新的途径。     

Expectations for Infrared Spectroscopy of 9P/Tempel 1 from Deep Impact

The science payload on the Deep Impact mission includes a 1.05–4.8 μm infrared spectrometer with a spectral resolution ranging from R∼200–900. The Deep Impact IR spectrometer was designed to optimize, within engineering and cost constraints, observations of the dust, gas, and nucleus of 9P/Tempel 1. The wavelength range includes absorption and emission features from ices, silicates, organics, and many gases that are known to be, or anticipated to be, present on comets. The expected data will provide measurements at previously unseen spatial resolution before, during, and after our cratering experiment at the comet 9P/Tempel 1. This article explores the unique aspects of the Deep Impact IR spectrometer experiment, presents a range of expectations for spectral data of 9P/Tempel 1, and summarizes the specific science objectives at each phase of the mission.     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

自适应直角切割网格民机增升装置绕流数值模拟

提出并介绍了基于直角切割网格的分区面搭接技术,采用变长宽比网格方法,成功地进行了存在外形间断(剪刀叉)的民机增升装置的网格生成和绕流Euler方程数值模拟.根据外形的特点,运用"根"网格分区算法,降低了整个网格的生成难度;通过基于外形的自适应网格加密技术,详细地描述了外形上的大量缝道和凹槽,提高了网格质量;在分区交界面上,利用重叠面积切割和面搭接算法实现了两侧网格间的流场信息传递,并保证了通量守恒;采用中心有限体积方法,结合双时间推进算法,完成流场的Euler方程数值模拟,计算结果与实验数据吻合良好,说明所述方法的正确性.     

关于三维Navier－Stokes方程的粘性项计算

借助于张量分析和张量计算，在贴体曲线坐标系下本文讨论了不同求解变量导致了粘性项个数上的重大差异和不同大小的计算量，并提出了便于粘性计算的最佳形式。文中借助于有限体积离散技术，通过引进两个对称辅助矩阵［Ａ］和［Ｂ］，使粘性项的计算量大大减少，这对完成三维粘性流的数值计算具有重要的指导意义。借助于上述方法，本文完成了某型真实进气道两种工况的三维粘性Ｎａｖｉｅｒ－Ｓｔｏｋｅｓ方程计算（即Ｍ∞＝３．０，α＝０°和设计工况Ｍ∞＝２．６５，α＝０°），获得了满意的全场结果；对于Ｍ∞＝２．６５的设计工况，同实验数据作了比较，符合良好。由于本文的方法明显的减少了粘性项的计算量且节省了大量内存，以致于使三维流场的Ｎ－Ｓ求解能在普通微机上进行。