中国中部低层大气行星波无线电探空仪的观测研究

通过分析武汉、宜昌和恩施气象局无线电探空仪2001-2003年的观测数据,研究了中国中部地区对流层和低平流层中行星波的特性.通过Lomb-Scargle(L-S)的周期图方法发现了周期为准16天和周期为准10天的谱分量占据着主导地位.观察发现,较大振幅的行星波振荡主要集中在5-15 km之间.准16天行星波沿纬圈向西传播,对应的纬圈波数大约为2,水平波长约为17 324.8 km,传播相速度约为-12.5 m·s-1(东向为正),通过计算准16天行星波在10 km以下相位随高度的改变可以得到其垂直波长大约为25-30 km,而在对波层顶附近其相位几乎没有发生改变,呈现出静态波特性.准10天行星波沿纬圈向东传播,对应的纬圈波数大约为4,水平波长约为8627.3 km,传播相速度约为10.0 m·s-1,垂直波长约为22-40 km.      

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。     

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。     

含C,Cr,Mo的Fe—10Ni—14Co钢的微观组织

用TEM对两种含碳量的高钴镍钢的微观组织进行了研究。结果表明,各状态试样组织中孪晶的出现,淬火温度、冷却速度的影响是次要的,与合金中的合金元素镍、铬、铜有更密切的关系。淬火+510℃回火5小时组织中除在淬火过程中形成的薄膜状残余奥氏体外,还存在穿板条及沿板条的呈片状或颗粒状的逆转变奥氏体,组织中的合金碳化物鉴定为Mo_2C。     

多线程异地备份发动机数据软件设计与应用

通过开发发动机信息管理系统后台数据的异地备份软件,介绍了以Delphi 10 Seattle为开发工具,应用Indy组件,多线程方式实现客户端向服务器端发送备份指令,完成数据的备份、加密压缩以及向异地客户端推送数据,以客户端完成压缩数据的接收结束异地传输,同时服务器端实时向不同客户端发送执行过程信息.因发动机数据量较大,备份和传输时间较长,在异地客户端采用同步进度条显示.软件设计采用TCP可靠传输,提高数据传输的安全性.