三维非平面裂纹扩展参数化模拟方法

发展一种基于有限元方法（FEM）的自动模拟三维非平面裂纹扩展的模拟方法。该方法采用参数化建模的方式建立裂纹体,以镶嵌裂纹体的方式在结构中插入裂纹,然后通过有限元计算得到裂纹扩展参量,自动更新裂纹体从而模拟裂纹的扩展过程。通过模拟三个裂纹扩展算例,计算了裂纹扩展循环数,对比试验结果,误差分别为195%、161%、21%。结果表明:该方法能够模拟三维非平面裂纹的扩展并计算扩展寿命,具有一定的精度和适用性。      

基于结构健康监测的飞机结构 MSG-3 分析

结构健康监测(SHM)技术被广泛引入到了飞机设计与维护,本文依据现阶段SHM技术的发展现状,将SHM技术与MSG-3分析思想融合,制定了一种针对采用SHM技术飞机结构的计划维修分析流程。     

三维夹层结构复合材料的制备及性能

采用酚醛树脂、氰酸酯树脂分别与三维中空芯层结构材料进行复合,制备不同树脂基三维中空芯层结构复合材料,对不同基体复合材料的力学及介电性能进行研究。结果表明,三维中空芯层结构与树脂复合工艺性良好,压缩强度达到5.0和3.5 MPa,与传统的蜂窝、泡沫材料相比,复合材料的力学性能得到较大幅度提高;介电常数为1.5和1.6,且在不同频率下显示优异的稳定性。     

吸热型碳氢燃料RP-3替代模型研究

利用广义对应态法则对吸热型碳氢燃料RP-3的5种替代模型的密度、黏度、导热系数和比定压热容进行了数值计算.计算温度变化范围为300~800K,压力变化范围为3~6MPa.结果表明:不同替代模型均能定性重现RP-3在拟临界温度附近的物性急剧变化;由53%正十一烷,18%正丁基环己烷,29%1,3,5-三甲基苯组成的3组分替代模型在预测RP-3物性上表现最优,相对于实验数据,300~700K内密度相对误差均小于0.08;替代模型的相对分子质量越大,预测的拟临界温度越高,对拟临界温度下物性值的影响无显著规律.      

Nb/Nb5Si3微叠层材料及其制备技术

Nb/Nb5Si3合金是未来最具潜力的超高温结构材料,实现该材料的结构微叠层化是一种新颖的材料设计思路和制备方法.Nb/Nb5Si3微叠层材料是将Nb和Nb5Si3按一定的层间距及层厚比以ABABAB型交互重叠结构形成的多层材料,其几种典型的制备技术包括热压、等离子喷涂、磁控溅射和电子束物理气相沉积(EB-PVD).其中EB-PVD是一种最适合工程应用的Nb/Nb5Si3微叠层材料制备方法,结构和功能复合、纳米化叠层、高韧化工艺是EB-PVD技术制备Nb/Nb5Si3微叠层材料的发展方向.     

飞机维修大纲中的任务转移风险评估方法

以波音737NG飞机维修大纲为例,对其依据MSG—3决断逻辑制定的维修大纲中的任务转移风险进行模糊综合评价。使用模糊理论、层次分析法、熵权法和转移修正因子计算维修大纲中任务转移的风险概率值。结果表明,该值符合FAA和EASA的安全标准,方法可行。     

高性能纤维增强树脂基复合材料3D打印及其应用探索

纤维增强树脂基复合材料具有优异的力学性能,能够实现轻质、高性能结构的制造,但传统的成型工艺过程复杂、成本高,难以实现纤维回收利用,限制了纤维增强树脂基复合材料的广泛应用.3D打印技术是一种新兴的零件成形工艺,将3D打印技术应用于纤维增强树脂基复合材料的制造,为实现复合材料低成本、绿色制造提供了可能性.综述了纤维增强树脂基复合材料3D打印技术研究的发展现状,提出了一种高性能连续纤维增强热塑性复合材料3D打印工艺及其回收再制造策略.     

A 3NM-64_He added to LARC for Solar Extreme Event studies during solar cycle 24

The Antarctic Laboratory for Cosmic Rays (LARC, acronym for Laboratorio Antartico per i Raggi Cosmici or Laboratorio Antártico para Rayos Cósmicos) operates on King George Island (South Shetlands). Since January 1991 a standard 6NM-64 detector has been recording continuous cosmic ray measurements and several Ground-Level Enhancements have been registered. Here we describe the different phases performed in Italy for the realization of a 3NM-64_³He detector, which started its measurements during the Italian XXII Antarctic Summer Campaign. Data recorded during solar activity cycle 24 will furnish an useful research tool for the next Solar Extreme Events.     

Orbital phase spectroscopy of four high mass X-ray binary pulsars to study the stellar wind of the companion

Our work focuses on a comprehensive orbital phase-dependent spectroscopy of the four High Mass X-ray Binary Pulsars (HMXBPs) 4U 1538-52, GX 301-2, OAO 1657-415 and Vela X-1. We hereby report the measurements of the variation of the absorption column density and iron-line flux along with other spectral parameters over the binary orbit for the above-mentioned HMXBPs in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. Out of the four pulsars, only in 4U 1538-52, we find the model having a reasonable corroboration with the observations, whereas in the remaining three the stellar wind seems to be clumpy and a smooth symmetric stellar wind model appears to be quite inadequate in explaining the data. Moreover, in GX 301-2, neither the presence of a disk nor a gas stream from the companion was validated. Furthermore, the spectral results obtained in the case of OAO 1657-415 and Vela X-1 were more or less similar to that of GX 301-2.