铸造K4169合金晶粒细化的研究

选用Ｋ４１６９铁－镍基高温合金研究了向熔体中加入ＮｉｘＡｌｙＴｉｚ金属间化合物对合金冷凝后的晶粒尺寸、枝晶组织等凝固组织特征的影响。结果发现,加入微量ＮｉｘＡｌｙＴｉｚ细化剂并控制合金液的均匀化处理过程可显著细化晶粒,将Ｋ４１６９铸件整体晶粒细化至０．１～０．２ｍｍ,达到ＡＳＴＭ１～３级,同时,枝晶组织和ＭＣ型碳化物也有明显变化。而且,本研究选用的ＮｉｘＡｌｙＴｉｚ细化剂由于其成分特点对合金的结晶特性及凝固组织无不良影响。因此可认为,加入微量的ＮｉｘＡｌｙＴｉｚ细化剂是获得Ｋ４１６９高温合金细晶铸件的有效方法。     

服务网格中面向业务用户的服务组合方法

服务网格环境中如何快速构建组合服务,为业务用户提供快速整合资源、配置集成化应用的平台,按需创建个性化应用,以降低大规模软件开发的成本、提高效率,成为了服务网格领域亟待解决的一个问题。提出了一种服务网格环境中面向业务用户的服务组合方法,它通过服务映射机制实现从业务用户所熟悉的业务服务到具体物理服务的映射;利用基于上下文的流程推导技术实现了组合业务服务流程向组合物理服务流程的映射;利用物理服务选取技术,生成能够最大限度满足用户需要的组合服务。研究表明该方法应用的原型系统,适用于普通业务用户,能够提高组合物理服务流程构建的效率。     

淬火／回火热处理对TiAl基合金晶粒细化的影响

研究了淬火/回火热处理中淬火温度和回火时间对Ti-48Al-2Cr-0.5Mo合金晶粒细化的影响。研究表明:一定的淬火/回火热处理能将大小约为1000μm的铸态组织细化成为18～30μm的均匀双态组织;TiAl基合金的细化效果严重依赖淬火阶段的加热温度,温度升高,得到的块状组织较细,羽毛状组织体积分数减少,在两相区回火时,高温淬火组织的回火组织较细,而时间的延长,晶粒长大,但不明显。     

网格技术及其在制造领域的应用

简要介绍了网格的概念、组成及其特征 ;结合当前制造业的发展趋势 ,对网格技术作了剖析 ,着重提出了网格技术在制造业中的应用模式和预期效果 ,指出制造网格是先进制造技术的发展方向     

高亚声速压气机叶片优化设计

为实现压气机叶片的优化设计,采用Hicks Henne函数进行叶型参数化,N S方程流场计算与混合遗传算法结合构成设计软件。以给定叶片表面压力分布为目标,以损失小而扩压度大和给定压比损失最小作为目标,所得优化叶片吸力面等熵马赫数分布合理、符合控制扩散规律,具有较好的压比和损失指标。采用几何方法与椭圆型方程方法结合生成壁面正交H型网格,可提高计算精度和便于采用代数紊流模型的流场计算。     

PIC16F877实现CAN总线分布式数据采集系统

叙述了一种采用CAN总线通信来实现分布式数据采集的设计方法;介绍了用PIC16F877通过SPI方式直接对MCP2510进行操作,与带智能适配卡的PC机实现CAN通信,并对CAN控制器MCP2510作了分析;给出了系统结构框图与部分硬件图,以及给出了软件设计思路。该基于CAN总线的分布式数据采集系统是一种高可靠性、实时性的系统。     

两种椭圆型方程求源项方法在喷管内流场网格生成中的应用

用椭圆型方程生成二维网格，发展两种Hilgenstock求源项方法，实现对网格与边界间距及与边界正交的控制。     

添加微量Sc对Mg-3Li合金高应变率变形行为的影响

利用Hopkinson压杆对Mg-3Li和Mg-3Li-1Sc合金进行了高应变率冲击实验,分析了添加少量Sc对Mg-3Li合金冲击变形行为及其应变率效应的影响.结果表明,在1350s～3000s-1应变率范围内,两种合金的动态应力-应变行为均表现出显著的应变率强化效应.但随应变率继续升高,合金的动态变形行为转为应变率弱...     

A fast and automatic full-potential finite volume solver on Cartesian grids for unconventional configurations

To meet the requirements of fast and automatic computation of subsonic and transonic aerodynamics in aircraft conceptual design,a novel finite volume solver for full potential flows on adaptive Cartesian grids is developed in this paper.Cartesian grids with geometric adaptation are firstly generated automatically with boundary cells processed by cell-cutting and cell-merging algo rithms.The nonlinear full potential equation is discretized by a finite volume scheme on these Cartesian grids and iteratively solved in an implicit fashion with a generalized minimum residual (GMRES) algorithm.During computation,solution-based mesh adaptation is also applied so as to capture flow features more accurately.An improved ghost-cell method is proposed to implement the non-penetration wall boundary condition where the velocity-potential of a ghost cell is modified by an analytic method instead.According to the characteristics of the Cartesian grids,the Kutta condition is applied by specially computing the gradients on Kutta-faces without directly assigning the potential jump to cells adjacent wake faces,which can significantly improve the solution con verging speed.The feasibility and accuracy of the proposed method are validated by several typical cases of sub/transonic flows around an ONERA M6 wing,a DLR-F4 wing-body,and an unconventional figuration of a blended wing body (BWB).The validation cases demonstrate a fast convergence with fully automatic grid treatment and computation,and the results suggest its capacity in application for aircraft conceptual design.     

A Parallel Adaptive 3D MHD Scheme for Modeling Coronal and Solar Wind Plasma Flows

A parallel adaptive mesh refinement (AMR) scheme is described for solving the governing equations of ideal magnetohydrodynamics (MHD) in three space dimensions. This solution algorithm makes use of modern finite-volume numerical methodology to provide a combination of high solution accuracy and computational robustness. Efficient and scalable implementations of the method have been developed for massively parallel computer architectures and high performance achieved. Numerical results are discussed for a simplified model of the initiation and evolution of coronal mass ejections (CMEs) in the inner heliosphere. The results demonstrate the potential of this numerical tool for enhancing our understanding of coronal and solar wind plasma processes. This revised version was published online in June 2006 with corrections to the Cover Date.