冷却速率、保温时间对DD3单晶合金TLP连接接头组织和性能的影响

对DD3单晶合金进行1250℃保温不同时间的TLP扩散连接研究。降温过程采取了随炉冷却和充氩快冷两种方式,随后对接头进行了870℃/32h/空冷的时效处理。分析了不同规范下的焊缝及母材的组织,同时测定了接头的980℃持久性能。结果发现:炉冷并时效处理试样的焊缝及母材中的γ'相的尺寸随着保温时间增加而增加,且形状趋于不规则。而充氩冷却并时效处理试样的焊缝及母材中的γ'相的尺寸和形状基本一致,随保温时间的增加没有明显变化,立方化较好。低的冷却速率使焊缝和母材中的γ'相粗化从而降低了接头和母材的性能,而高的冷却速率促使焊缝及母材中形成细小立方化的γ'相,不仅使接头性能明显提高,同时母材性能也没有降低。     

钛合金超塑成型/扩散连接舵面颤振设计

钛合金超塑成型/扩散连接结构是一种新型的结构形式。以某型空空导弹舵面结构为实例,对钛合金超塑成型/扩散连接舵面颤振建模和设计进行了研究。采用有限元软件,计算和分析了舵面气动外形、舵面重心对颤振特性的影响,确定了满足导弹颤振裕度要求的舵面结构形式。     

推进剂功能组分作用研究(Ⅲ)--聚醚/硝酸酯体系

在硝酸酯增塑的聚醚粘合剂与HMX、AP、Al固体组成的实验体系中，用流变学方法研究推进剂功能组分中性聚合物键合剂NPBA和MAPO的影响特征及作用机理。实验结果表明，NPBA明显增加HMX体系的粘度和屈服值，对HMX产生的可能是物理键合作用，其合适的加入量应为HMX重量的1．0％－1．5％，同时还存在作用的时间效应。实验还发现NPBA是粉碎细AP的优良工艺助剂，可大幅度降低粘度，其适宜加入量为细AP的0．4％。MPAO能对细AP起很好的界面改性作用，显著改善推进剂药浆的工艺性能。但MAPO、NPBA对铝粉无明显作用。     

刚度不平衡胶合接头的分析

对具有不同弹性模量、不同厚度的两种材料之间的胶合接头进行了分析。在Ｇ－Ｒ理论的基础上推导了接头胶层应力微分方程及通过实例计算对这种刚度不平衡的接头胶层应力分布进行了分析;讨论了被接件刚度不平衡程度对胶层应力分布的影响。     

新型中性聚合物键合剂设计与合成

首先以三-(2-甲基氮丙啶基)氧化膦(MAPO)与丙烯酸(AA)为原料合成MAPO的衍生物,通过红外和质谱对产物进行了定性分析,用非水滴定的方法检测氮丙啶环的含量,通过正交试验设计得到了较优工艺条件:MAPO与AA的摩尔比为1:1,反应温度为70 ℃,反应时间为2.5 h,所得氮丙啶环含量最接近理论值.再利用该活性中间体与丙烯腈、丙烯酸羟乙酯共聚,得到改性的中性聚合物键合剂,通过接触角的测量,粘接性能预估表明,该新型中性聚合物键合剂与黑索金(RDX)、奥克托金(HMX)、高氯酸铵(AP)的界面浸润好、粘接强.     

钛合金典型连接结构裂纹扩展特性分析

基于扩展有限元方法研究钛合金传统机加接头耳片与含预置非焊合区的层合接头耳片结构在拉-拉疲劳荷载作用下的裂纹扩展特性,揭示螺栓孔在受挤压情况下非焊合区对钛合金典型连接结构疲劳裂纹扩展的抑制作用,并通过试验验证扩展有限元方法对钛合金典型连接耳片结构裂纹扩展特性分析的有效性。     

MGH956合金TLP扩散连接接头组织分析

研制了合适的中间层合金KCo2,采用过渡液相(简称TLP)连接方法进行扩散连接试验,分析接头显微组织、成分和连接工艺的关系,分析焊接缺陷形成原因,确定了MGH956合金TLP扩散连接机理.结果表明在1240℃,保温8小时条件可以获得焊接缺陷少,连续完整的焊接接头.元素实现扩散均匀化.     

风扇进气道胶接蜂窝声衬样件声学性能实验研究

使用消声短舱是降低飞机噪声的重要方法。本文介绍的高速压气机实验台架消声短舱样件的声学实验在以往基础上进行改进 ,增加了消声终端 ,使用可工程应用的胶接铝蜂窝制作的进气道消声短舱原理样件 ,测量了各压气机工况下声衬的减噪量和总压损失。测量结果表明漏气增加了总压损失 ,某些声衬组合可明显增加减噪量     

Transient Effects and Disturbed Conditions

In the present phase of the solar cycle no big transients leading to strong modulation had been observed after 1991. Apart from a few minor disturbances cosmic rays were still recovering to a new intensity maximum. It was suggested, therefore, that existing literature from previous cycles should be critically reviewed. The scene was set by the introductory papers on— phenomenology of cosmic ray modulation in successive solar cycles throughout the heliosphere— the present state of models for long term modulation and their shortcomings— the relation between cosmic ray variations and the magnitude of the interplanetary magnetic field (the CR-B-relation)— charge dependent effects.In the discussions, the study of propagating diffusive disturbances and the CR-B-relation played a central role. The difference was stressed between isolated transient disturbances in the inner solar system (Forbush decreases), and the long lasting, step-like decreases caused by merged interaction regions in the outer heliosphere. The recovery rates following the step-like decreases vary with the phase in the 22-year solar cycle. In some cases this requires a modification of existing drift models. In the outer heliosphere, the CR-B-relation leads to the result 1/ between the diffusion coefficient and the field magnitude . This simple result is a challenge for theoreticians to derive the perpendicular diffusion coefficient fromfirst principles. The three articles in this report essentially follow the list of open points and arguments just presented.The article "Observations and Simple Models" is organised around the model of a propagating diffusive barrier, its application to Forbush effects in the inner heliosphere and to decreases caused by merged interaction regions in the outer heliosphere. Acomparison of observed Forbush decreases with model predictions requires a careful separation of the two steps related to the turbulent region behind the shock front and the closed magnetic field regions of the ejecta (the interplanetary counterparts of coronal mass ejections). It is shown that models for propagating disturbances can be used to derive values of the diffusion coefficients phenomenologically, not only during the disturbance, but also in the ambient medium.The "Modeling of Merged Interaction Regions" summarizes the dynamic and time-dependent process of cosmic ray modulation in the heliosphere. Numerical models with only a time-dependent neutral sheet prove to be successful when moderate to low solar activity occurs but fail to describe large and discrete steps in modulated cosmic rays when solar activity is high. To explain this feature of heliospheric modulation, the concept of global merged interaction regions is required. The com-bination of gradient, curvature and neutral sheet drifts with these global merged interaction regions has so far been the most successful approach in explaining the 11-year and 22-year cycles in the long-term modulation of cosmic rays.The "Remarks on the Diffusion Tensor in the Heliosphere" describe available theories of perpen-dicular diffusion and drift, and discuss their relevance to cosmic rays in the heliosphere. In addition, the information about diffusion coefficients and spatial gradients obtained from the analysis of steady state anisotropies at neutron monitor energies is summarized. These topics are intimately related to the other two articles. They are also part of the general discussion about the "Diffusion Tensor throughout the Heliosphere" which played an important role in all working groups.     

B/Al复合板材复合工艺的研究

介绍了热压扩散结合法制备Ｂ／Ａｌ复合板材的工艺过程,研究了热压工艺参数对Ｂ／Ａｌ复合板材性能的影响,获得了热压扩散结合法制备Ｂ／Ａｌ复合板材比较理想的工艺参数,得到了拉伸强度σｂ＝１２８０ＭＰａ、弹性模量Ｅ＝２３３ＧＰａ的Ｂ／Ａｌ复合板材。