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。     

300M钢纯洁度磁粉检验磁痕现象的分析

采用交、直流磁粉检验并结合金相试验、电子探针试验及微量元素含量分析的方法，对３００Ｍ钢磁痕现象的本质进行了分析。结果表明，采用磁粉检验方法对航空优质钢进行纯洁度检验是可信的。     

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.     

应用声发射技术实时监测某型机防扭支架疲劳试验裂纹

随着声发射技术的发展,声发射技术在工程无损检测上的运用日益广泛。本文对声发射技术的应用现状、基本理论及在直升机某型机防扭支架疲劳试验裂纹监测中的应用进行了介绍。希望通过应用声发射技术,能及时捕捉疲劳裂纹形成和扩展的过程,给判定疲劳试验件是否破坏带来更准确、客观的依据,从而能为直升机动部件和结构件的准确定寿提供一种科学的辅助手段。     

轻金属颗粒燃烧理论研究进展

介绍了铝、镁和铍一类轻金属颗粒在氧化氛围中燃烧的有关实验现象，并在此基础上对蒸气相扩散机理、多相机理及复合机理进行了述评。     

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.     

粒子云侵蚀问题实验研究中动能通量模拟的意义

本文首先将粒子云侵蚀条件下的驻点表面后退分解为无粒子烧蚀部分、粒子云引起的烧蚀增量部分和粒子撞击物面引起的直接侵蚀部分。然后研究了表面能量平衡关系,给出了粒子云引起的烧蚀增量表达式。最后分三类讨论粒子与飞行器的碰撞:(1)完全弹性碰撞(不符合实际);(2)完全非弹性碰撞;(3)部分弹性碰撞。对于后两种碰撞,本文分析了动能通量模拟适用的条件。     

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。     

激波作用下粉尘卷扬,点火与燃烧的数值研究

根据本文给出的守恒方程和计算方法，对激波与沉积可燃粉尘的相互作用进行了数值研究，讨论了激波作用下的颗粒的上扬、点火与燃烧的基本特征以及波后燃烧粉尘云的内部结构。     

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.