TC4钛合金的微动磨损及防护

对Ｔｉ－６Ａｌ－４Ｖ合金在１８℃，１００℃２５０℃下的微动磨损特性及防护工艺进行了研究。表明：该合金微动磨损的主要磨损形式是疲劳脱层，其磨损量随温度升高而下降，高渐微动磨损量与磨损区表面所形成的氧化层的性质及厚度有关。     

离散系统仿真输出数据的统计分析

概括了分析仿真产生的数据的方法，讨论了离散系统仿真输出分析的目的以及应用统计方法的要求，对单变量情形，给出了有关估计来自终态仿真和和稳态仿真参数的技术。对多变量情形，以终态仿真为例，给出了用于分析离散系统的仿真输出的某些多变量统计技术，并提出均值向量的估计方法。     

空间碎片防护结构设计优化理论方法研究

航天器空间碎片防护结构设计优化在国际上属前沿课题，防护结构设计优化理论方法是其关键技术之一。在防护优化理论模型及其优化算法研究方面取得了突破性进展，建立了综合各类典型防护结构构型的统一的防护优化数学模型，提出了解决防护优化问题的几种算法：混合遗传算法，改进的差异演化算法和混合差异演化算法。最后采用航天器防护优化算例对防护优化理论方法进行了测试考核，优化结果表明了本文工作的可行性和有效性。     

建立民航维修专家系统的分析

简要介绍了专家系统的原理及构成.分析了“设计民航维修专家系统”的过程,目前加拿大正着手研制的“先进的维修软件系统”的概况.最后提出专家系统需要解决的关键技术问题及发展情况.     

High Excitation ISM and Gas

An overview is given of ISO results on regions of high excitation ISM and gas, i.e. HII regions, the Galactic Centre and Supernova Remnants. IR emission due to fine-structure lines, molecular hydrogen, silicates, polycyclic aromatic hydrocarbons and dust are summarised, their diagnostic capabilities illustrated and their implications highlighted. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

逻辑分析仪部分参数测量结果的不确定度评定

介绍了逻辑分析仪部分参数测量结果的不确定度分析评定方法，评定过程及结论，可应用在对于计量标准进行相应指标的不确定度评定分析上。     

用于棘轮变形预测的棘轮演化统一模型研究

 在大量单轴棘轮实验基础上,研究了均值、幅值、峰值和谷值应力对 304不锈钢的饱和棘轮应变的影响规律,首次提出了棘轮应力σ_r和棘轮门槛值σ_rth 的概念,建立了基于单参数控制的、用于饱和棘轮应变预测的 SRM饱和棘轮本构模型和用于独立循环应力工况下棘轮应变演化预测的 REM棘轮演化模型,并由此发展了全面描述任意循环应力工况下棘轮应变演化规律的 URM棘轮演化统一模型。抛物律模型 SRM和幂律模型 REM对实验数据拟合的相关系数均超过 0.98。URM建模容易,只需 4～ 6个试样的单轴棘轮实验数据。此外还讨论了获得 SRM本构模型的单试样实验法。     

Evolution of the Protosolar Nebula and Formation of the Giant Planets

The formation of planetary systems is intimately tied to the question of the evolution of the gas and solid material in the early nebula. Current models of evolution of circumstellar disks are reviewed here with emphasis on the so-called “alpha models” in which angular momentum is transported outward by turbulent viscosity, parameterized by an dimensionless parameter α. A simple 1D model of protoplanetary disks that includes gas and embedded particles is used to introduce key questions on planetesimal formation. This model includes the aerodynamic properties of solid ice and rock grains to calculate their migration and growth. We show that the evolution of the nebula and migration and growth of its solids proceed on timescales that are generally not much longer than the timescale necessary to fully form the star-disk system from the molecular cloud. Contrary to a widely used approach, planet formation therefore can neither be studied in a static nebula nor in a nebula evolving from an arbitrary initial condition. We propose a simple approach to both account for sedimentation from the molecular cloud onto the disk, disk evolution and migration of solids. Giant planets have key roles in the history of the forming Solar System: they formed relatively early, when a significant amount of hydrogen and helium were still present in the nebula, and have a mass that is a sizable fraction of the disk mass at any given time. Their composition is also of interest because when compared to the solar composition, their enrichment in elements other than hydrogen and helium is a witness of sorting processes that occured in the protosolar nebula. We review likely scenarios capable of explaining both the presence of central dense cores in Jupiter, Saturn, Uranus and Neptune and their global composition. This revised version was published online in August 2006 with corrections to the Cover Date.     

数控展成电解加工的阴极结构及流场研究

介绍了应用数控展成电解在整体叶轮毛坯上开槽时的流场特点,讨论了阴极结构对加工间隙内流场的影响规律,并相应对阴极的结构设计提出了一些建议。     

数控展成电解磨削整体叶轮叶片的过切误差分析及解决方案

分析了平行直纹展成电解磨削整体叶轮叶片的过切误差,得到了过切误差计算公式,提出了用圆锥磨轮和组合式五轴联动数控方案来消除过切误差的方法。