Dynamic tensile behavior of AZ31B magnesium alloy at ultra-high strain rates

The samples having {0001} parallel to extruding direction(ED) present a typical true stress–true strain curve with concave-down shape under tension at low strain rate. Ultra-rapid tensile tests were conducted at room temperature on a textured AZ31 B magnesium alloy. The dynamic tensile behavior was investigated. The results show that at ultra-high strain rates of 1.93 · 102 s 1and 1.70 · 103 s 1, the alloy behaves with a linear stress–strain response in most strain range and exhibits a brittle fracture. In this case, {10-12} 10-11 extension twinning is basic deformation mode. The brittleness is due to the macroscopic viscosity at ultra-high strain rate, for which the external critical shear stress rapidly gets high to result in a cleavage fracture before large amounts of dislocations are activated. Because {10-12} tension twinning, {10-11} compressive twinning,basal a slip, prismatic a slip and pyramidal c + a slip have different critical shear stresses(CRSS), their contributions to the degree of deformation are very differential. In addition,Schmid factor plays an important role in the activity of various deformation modes and it is the key factor for the samples with different strain rates exhibit various mechanical behavior under dynamic tensile loading.     

电化学辅助沉积KH-570硅烷对AZ31B镁合金耐蚀性能的影响

采用电化学辅助沉积方法对AZ31B镁合金进行硅烷化处理,借助于动电位极化曲线和电化学阻抗谱等电化学测试手段研究了γ-(甲基丙烯酰氧基)丙基三甲氧基硅烷(KH-570)添加量对膜层质量及耐蚀性能的影响,并比较了利用羟基磷灰石(HA)颗粒、铈盐离子(Ce3+)两种改性物质改良硅烷溶液后所制得膜层的质量及耐蚀性能.结果表明:AZ31B镁合金经电化学辅助沉积硅烷处理后,表面生成一层均匀而致密的硅烷透明膜层,有效地减缓了镁合金的腐蚀行为,促使其自腐蚀电流密度大大降低;在硅烷电化学辅助沉积处理过程中,KH-570存在最佳添加量,当其添加体积约为8 mL时所制备出的硅烷膜层质量最好、耐蚀性能最佳;通过改良硅烷溶液,电化学辅助沉积制备的硅烷膜层质量进一步提高,Ce3+改良效果更佳.     

基于ECSS标准的航天器姿轨控系统内1553B总线数据协议设计

摘要： 国内外航天器姿轨控系统广泛应用基于1553B内总线的体系结构.针对国内航天器姿轨控系统内部1553B总线数据协议不统一带来的可集成性、可扩展性和通用性差的问题，本文设计了基于ECSS标准的姿轨控系统内1553B数据总线协议，从姿轨控系统内部总线数据业务需求分析出发，提出了四层结构的数据协议体系结构，重点介绍了在应用支持层和链路服务层应用ECSS标准的总线协议设计，并说明了协议的应用情况.应用该国际通用的标准协议，有助于实现国内航天器姿轨控系统内1553B总线数据协议的标准化，进而提升姿轨控系统体系结构的可集成性、可扩展性、以及星载设备(含软件)的通用化.     

某型飞机典型结构应力腐蚀开裂原因分析

针对某型飞机典型结构应力腐蚀开裂问题,从材料选用、结构加工、装配工艺、服役环境等角度,结合有限元模拟细节应力分析技术,分析了发生应力腐蚀开裂的原因。基于分析结果,为新飞机制造和现役飞机维修提供相应的建议,为制造厂和维修厂提高飞机结构的应力腐蚀抗性以及结构完整性和航空安全性提供参考。     

浅析由磁条引发的乘务内话重复故障的排除

针对一起波音737NG飞机乘务话筒内话重复故障，通过观察分析、串件对比核实，确定故障原因为磁条松动，并进行了彻底排除。     

New insights into SNR evolution revealed by the discovery of recombining plasmas

We report the discovery of recombining plasmas in three supernova remnants (SNRs) with the Suzaku X-ray astronomy satellite. During SNR’s evolution, the expanding supernova ejecta and the ambient matter are compressed and heated by the reverse and forward shocks to form an X-ray emitting hot plasma. Since ionization proceeds slowly compared to shock heating, most young or middle-aged SNRs have ionizing (underionized) plasmas. Owing to high sensitivity of Suzaku, however, we have detected radiative recombination continua (RRCs) from the SNRs IC 443, W49B, and G359.1–0.5. The presence of the strong RRC is the definitive evidence that the plasma is recombining (overionized). As a possible origin of the overionization, an interaction between the ejecta and dense circumstellar matter is proposed; the highly ionized gas was made at the initial phase of the SNR evolution in dense regions, and subsequent rapid adiabatic expansion caused sudden cooling of the electrons. The analysis on the full X-ray band spectrum of IC 443, which is newly presented in this paper, provides a consistent picture with this scenario. We also comment on the implications from the fact that all the SNRs having recombining plasmas are correlated with the mixed-morphology class.     

波音737系列飞机结构修理类型分类方法

根据FAA颁发的AASR的要求,2010年12月20日以后,波音737-系列飞机的维护计划中需包含损伤容限的基本检查要求。波音依据AASR的要求对需要进行损伤容限分析的结构修理的批准实施了新的方法。新方法的实施,导致波音对结构修理类型分类法方法和批准方式的改变。     

基于CORBA的分布式数据业务管理系统的设计和实现

概要介绍分布式数据业务管理系统的主要功能,展示基于CORBA的多层B/S结构和导构环境下对象的集成、主动服务、分布式事务和并发控制等.     

固体超强酸TiO2／SO4^2—催化合成苹果酯—B

使用ＴｉＯ２／ＳＯ４＾－２为催化剂，催化乙酰乙酸乙酯和１，２－丙醇反应合成苹果酯－Ｂ。结果表明：使用该催化剂１．０ｇ，乙酰乙酸乙酯（０．０７７ｍｏｌ）与１，２－丙二醇摩尔比为１：１．２，环已烷１５ｍｌ，反应２．５ｈ，苹果酯－Ｂ产率达７３％。产品经理化检验确认。     

Optical/infrared observations unveiling the formation,nature and evolution of High-Mass X-ray Binaries

In this review I first describe the nature of the three kinds of High-Mass X-ray Binaries (HMXBs), accreting through: (i) Be circumstellar disc, (ii) supergiant stellar wind, and (iii) Roche lobe filling supergiants.