近距离DPIV粒子成像分析

在PIV(Particle Image Velocimetry)近距离拍摄中,通过对在非傍轴成像条件下薄透镜成像公式的推导,求得粒子图像成像点的近似解析解,对粒子图像的成像位置在PIV图像计算中的影响作了讨论;同时也对已知直径粒子进行了试验拍摄,将试验所得的数据与理论推导的结果进行了比较,对在近距离拍摄中光圈对粒子成像的影响给出了定量分析.      

JSF战机动力装置研制新特点浅析

美国军方提出以现有发动机型号F119为基础来研制第四代轻型战机JSF,既降低了新机的技术风险,缩短型号研制周期,又可大幅度地节省项目研发资金和降低型号全寿命成本,这一思路值得关注或借鉴。通过对F-35战机基本型发动机F135和备用型F136发动机的最新发展动态分析,阐述了军用飞机动力装置类型从常规的涡喷/涡扇发动机向非常规的变循环发动机转变是一个必然发展趋势;而航空动力研制方法正从”传统设计”向更先进的”预测设计”过渡。     

不同中间层合金对IC10合金的连接

采用B或Zr作为降熔元素分别配制不同中间层合金,并对IC10合金进行连接.分析不同状态下焊缝组织.结果表明,含B中间层合金连接IC10时,保温时间较长可以达到等温凝固,而含Zr中间层合金在本试验条件下表现为钎焊过程.     

IC10单晶高温合金室温和750℃高周疲劳行为

在涡轮叶片服役过程中,疲劳是其失效的重要原因之一,而已有研究主要针对不同应变速率下IC10合金1 100℃低周疲劳性能展开,本文研究定向凝固IC10单晶高温合金静态空气介质环境下室温和750℃高周疲劳性能。在应力比R=-1、f≈83.3Hz条件下,进行高周疲劳试验,并利用扫描电镜对疲劳断口进行观察;基于试验观测结果,讨论室温和750℃下IC10单晶高温合金高周疲劳性能差异的内在机制。结果表明:IC10单晶室温疲劳强度为288 MPa,750℃疲劳强度为416 MPa;裂纹萌生于试样表面或近表面缺陷处,断口主要由裂纹萌生区、稳态扩展区和组成。     

钽钨合金表面铱涂层的制备及高温氧化性能

利用真空电弧离子沉积技术在钽钨合金表面沉积均匀致密的铱涂层,研究了钽钨合金/铱涂层的抗高温氧化性能和热震性能。结果表明:在800℃和1 100℃条件下,铱涂层可以有效保护钽钨合金,经过20 h后,铱涂层表面只发生轻微氧化,其表面形成褐色氧化铱产物;在1 900℃条件下,抗氧化寿命达10 h以上;在室温至(1 900±50)℃热震条件下,其寿命可达到1 000次以上。     

Z-A模型的修正及在预测本构关系中的应用

Zerilli-Armstrong(Z-A)模型是基于热激活位错运动理论建立的具有物理理论基础的本构模型,但是模型建立的初始假设,降低了其预测精度.为此通过引入考虑应变率和温度耦合效应的应变强化指数对Z-A模型进行修正,拓展了其适用范围,并将修正后的Z-A模型应用于描述IC10合金在不同温度和应变率条件下的塑性流变行为.与修正前Z-A模型的预测结果及试验结果比较表明:修正后Z-A模型的预测精度有较大程度的提高,最大平均相对误差值从6.41%降低到3.65%.      

The Geology of Mercury: The View Prior to the MESSENGER Mission

Mariner 10 and Earth-based observations have revealed Mercury, the innermost of the terrestrial planetary bodies, to be an exciting laboratory for the study of Solar System geological processes. Mercury is characterized by a lunar-like surface, a global magnetic field, and an interior dominated by an iron core having a radius at least three-quarters of the radius of the planet. The 45% of the surface imaged by Mariner 10 reveals some distinctive differences from the Moon, however, with major contractional fault scarps and huge expanses of moderate-albedo Cayley-like smooth plains of uncertain origin. Our current image coverage of Mercury is comparable to that of telescopic photographs of the Earth’s Moon prior to the launch of Sputnik in 1957. We have no photographic images of one-half of the surface, the resolution of the images we do have is generally poor (∼1 km), and as with many lunar telescopic photographs, much of the available surface of Mercury is distorted by foreshortening due to viewing geometry, or poorly suited for geological analysis and impact-crater counting for age determinations because of high-Sun illumination conditions. Currently available topographic information is also very limited. Nonetheless, Mercury is a geological laboratory that represents (1) a planet where the presence of a huge iron core may be due to impact stripping of the crust and upper mantle, or alternatively, where formation of a huge core may have resulted in a residual mantle and crust of potentially unusual composition and structure; (2) a planet with an internal chemical and mechanical structure that provides new insights into planetary thermal history and the relative roles of conduction and convection in planetary heat loss; (3) a one-tectonic-plate planet where constraints on major interior processes can be deduced from the geology of the global tectonic system; (4) a planet where volcanic resurfacing may not have played a significant role in planetary history and internally generated volcanic resurfacing may have ceased at ∼3.8 Ga; (5) a planet where impact craters can be used to disentangle the fundamental roles of gravity and mean impactor velocity in determining impact crater morphology and morphometry; (6) an environment where global impact crater counts can test fundamental concepts of the distribution of impactor populations in space and time; (7) an extreme environment in which highly radar-reflective polar deposits, much more extensive than those on the Moon, can be better understood; (8) an extreme environment in which the basic processes of space weathering can be further deduced; and (9) a potential end-member in terrestrial planetary body geological evolution in which the relationships of internal and surface evolution can be clearly assessed from both a tectonic and volcanic point of view. In the half-century since the launch of Sputnik, more than 30 spacecraft have been sent to the Moon, yet only now is a second spacecraft en route to Mercury. The MESSENGER mission will address key questions about the geologic evolution of Mercury; the depth and breadth of the MESSENGER data will permit the confident reconstruction of the geological history and thermal evolution of Mercury using new imaging, topography, chemistry, mineralogy, gravity, magnetic, and environmental data.     

16Co14Ni10Cr2Mo钢力学性能与应力腐蚀行为

研究了１６Ｃｏ１４Ｎｉ１０Ｃｒ２Ｍｏ钢不同温度回火５ｈ强度、冲击韧性、断裂韧性和应力腐蚀性能（在３．５％ＮａＣｌ水溶液中）。在５１０℃回火可以获得较高的强度，最高的断裂韧性及抗应力腐蚀性能，此时Ｋ＿（ＩＳＣＣ）可达，Ｋ＿（ＩＣ）为，屈服强度为１５８０ＭＰａ。应力腐蚀性能（ＳＣＣ）的改善主要与在较高温度回火，使Ｍｏ＿２Ｃ共格造成的应力下降，位错亚结构的恢复及碳化物的粗化，并导致氢的偏聚下降有关。     

一种较简单的低循环疲劳寿命预测法

 <正> 1。引言 局部应力应变法是目前预测结构裂纹起始寿命的一种行之有效的方法。根据局部应力应变法的原理,可以用计算的方法来预测构件裂纹起始寿命。在计算中,从载荷谱得到局部应变谱,可利用有限元法分析结构的局部应力应变响应。当然还可利用半经验公式(如Neuber法等)。在计算中若考虑材料的记忆特性和循环σ-ε曲线,这无疑对真实地反映受载构件的局部应力应变响应是有利的。但要做到这一点,用有限元分析所需的机时相当可观,因为它要对整个寿命期间的载荷历程进行分析计算,至少也要针对一个典型谱分析计算。 计算中材料的循环应力应变曲线一般可采用下式     

草酸钠体系中Ti-10V-2Fe-3Al钛合金阳极氧化膜的制备与表征

对Ti-10V-2Fe-3Al钛合金在草酸钠为主盐的新型无氟环保电解液体系中的阳极氧化进行了研究,成功制备出阳极氧化膜。采用扫描电子显微镜(SEM)、能谱仪(EDS)、X射线衍射仪(XRD)等仪器研究了氧化膜的形貌、组成和相结构。采用电化学方法研究了阳极氧化后钛合金的耐腐蚀性能。结果表明:膜层具有多孔结构,孔径范围在80nm～1μm之间。膜层的主要成分是无定形的TiO2,同时有锐钛矿相及金红石相TiO2的存在。阳极氧化后钛合金的耐蚀性有显著的提高。