Re对Ni3Al屈服强度及断裂强度影响的第一原理研究

为了满足航空发动机热端部件材料力学性能的不断提高,应用基于密度泛函理论的第一原理方法,研究了Re对Ni_3Al金属间化合物力学强度的影响。通过建立掺杂Re前后Ni_3Al的滑移模型和断裂模型,计算了晶胞的不稳定堆垛层错能γ_(US)和断裂能γ_C,进而判断Re对Ni_3Al屈服强度和断裂强度的影响。另外根据经验判据,γ_C/γ_(US)值可表征材料的韧脆性。计算结果表明,Re的掺杂增大了Ni_3Al [11■](111)和[1■0](111)两个滑移系下的γ_(US),使得滑移系不易开动,不易使Ni_3Al发生塑性变形,增大了Ni_3Al的屈服强度。Re增大了Ni_3Al在密排面处的断裂能,使得其不易在密排面发生断裂,增大了断裂强度。关于改善Ni_3Al的韧性,Re的掺杂对于密排面上不同滑移方向的影响具有一定的差别。此研究工作可为改善航空发动机单晶叶片的力学性能提供理论基础。     

压力和DNTF含量对DNTF-CMDB推进剂热分解动力学的影响

用高压差示扫描量热(PDSC)、热重等热(TG-DTG)分析技术,研究了不同压力和DNTF含量对4种DNTF-CMDB推进剂热分解行为及动力学的影响。结果表明,DNTF含量对CMDB推进剂的热分解特征量有明显影响,分解热ΔHd与ΔT的比值(ΔHd/ΔT)随DNTF加入量的增加而下降,同时DNTF的加入也影响PDSC和DTG的峰形。高压下DNTF-CMDB推进剂的活化能均较常压小,高压使初始分解的反应速率常数提高,且随DNTF含量增加,活化能逐渐增大,分解初始阶段反应速率常数减小,6 MPa下的结果与燃速随DNTF含量增加呈下降的趋势相一致。     

TiFe0．86Cr0．1／NaM复合贮氢材料的合成与性质

 利用蒸汽相法制备沸石技术合成ＴｉＦｅ０．８６Ｃｒ０．１／ＮａＭ复合贮氢材料的各种条件,找到了较适宜的碱度ＳｉＯ＿２／Ａｌ＿２Ｏ＿３以及合金与沸石。研究了合成条件对贮氢容量的影响,结果表明,沸石为单一晶相合成粒度不低于７４μｍ为佳。同时,该材料亦表现出良好的抗Ｏ＿２、ＣＯ＿２中毒特性。     

烧蚀反应动力学参数的确定

本文提出了一种理论模型与实验相结合确定碳基材料烧蚀反应动力学参数(活化能和指前因子)的方法。首先建立了碳基材料热化学烧蚀的湍流边界层模型,运用数值方法对边界层守恒方程组、表面烧蚀和固相热传导进行耦合求解,计算过程中不需要事先假设烧蚀的控制类型。其次,在电弧加热器中模拟火箭发动机喷喉的烧蚀环境进行烧蚀材料与氧化性气体反应的烧蚀实验。最后,运用所建立的模型和在电弧加热器上的实验结果进行预测比较,确定烧蚀反应的动力学参数。作为实例,确定了石墨与CO_2的烧蚀反应的动力学参数。     

聚合物基复合材料自修复体系的构成与修复机制分析

介绍了聚合物基自修复复合材料的分类、构成及自修复机制,以被动模式的埋植式修复体系为重点进行了详细的分析.在此基础上,提出了一种新的被动模式自修复体系设计.     

先进复合材料国防科技重点实验室的航空树脂基复合材料研发进展

归纳先进复合材料国防科技重点实验室在航空先进树脂基复合材料方面的应用和研究进展.研制出超薄热塑性无纺织物层间增韧技术以实现提高复合材料的CAI性能.设计出的多夹层结构具有多层吸收拓展频带的作用,使多夹层隐身复合材料的吸收频宽达1 ～ 18GHz.高韧性树脂基复合材料和耐高温复合材料技术得到发展,并形成预浸料-热压灌成型、液态成型和自动化制造技术体系.发展复合材料固化、树脂流动、固化变形等模拟优化技术,并建立复合材料数据库技术.建立先进复合材料国防科技重点实验室可在支撑航空装备研制,在航空复合材料创新引领、体系主导、基础支撑和保障应用方面发挥作用.     

高校分析化学人才培养模式研究

高校是分析化学人才培养的摇篮,然而,目前高校分析化学人才培养中存在诸多问题,使得高校难以顺应时代对分析化学人才的需求。为此,分析了21世纪分析化学人才应该具备的素质,并以此为基点,探讨了目前高校分析化学人才培养的误区,提出分析化学人才培养模式的调整思路。     

Inflatable shape changing colonies assembling versatile smart space structures

Various plants have the ability to follow the sun with their flowers or leaves during the course of a day via a mechanism known as heliotropism. This mechanism is characterised by the introduction of pressure gradients between neighbouring motor cells in the plant?s stem, enabling the stem to bend. By adapting this bio-inspired mechanism to mechanical systems, a new class of smart structures can be created. The developed overall structure is made up of a number of cellular colonies, each consisting of a central pressure source surrounded by multiple cells. After launch, the cellular arrays are deployed in space and are either preassembled or alternatively are attached together during their release or afterwards. A central pressure source is provided by a high-pressure storage unit with an integrated valve, which provides ingress gas flow to the system; the gas is then routed through the system via a sequence of valve operations and cellular actuations, allowing for any desired shape to be achieved within the constraints of the deployed array geometry. This smart structure consists of a three dimensional adaptable cellular array with fluid controlling Micro Electromechanical Systems (MEMS) components enabling the structure to change its global shape. The proposed MEMS components include microvalves, pressure sensors, mechanical interconnect structures, and electrical routing. This paper will also give an overview of the system architecture and shows the feasibility and shape changing capabilities of the proposed design with multibody dynamic simulations. Example applications of this lightweight shape changing structure include concentrators, mirrors, and communications antennas that are able to dynamically change their focal point, as well as substructures for solar sails that are capable of steering through solar winds by altering the sails? subjected area.     

三氢化铝的合成及性能研究

采用LiAlH4还原AlCl3的方法制备了AlH3,产品的产率大于90%。采用不同的稳定剂对合成的样品进行了稳定化处理,将经处理的样品通过在70℃进行放气量测试比较了热稳定性,发现经稀酸处理的AlH3样品稳定性最好。研究了AlH的安全性能,并通过DSC法研究了AlH与常用推进剂组分的相容性。     

Coupled Clouds and Chemistry of the Giant Planets— A Case for Multiprobes

In seeking to understand the formation of the giant planets and the origin of their atmospheres, the heavy element abundance in well-mixed atmosphere is key. However, clouds come in the way. Thus, composition and condensation are intimately intertwined with the mystery of planetary formation and atmospheric origin. Clouds also provide important clues to dynamical processes in the atmosphere. In this chapter we discuss the thermochemical processes that determine the composition, structure, and characteristics of the Jovian clouds. We also discuss the significance of clouds in the big picture of the formation of giant planets and their atmospheres. We recommend multiprobes at all four giant planets in order to break new ground.