工件淬火过程表面综合换热系数的测算

表面换热系数是温度场计算中一个重要参数,它的取值将直接影响到温度场计算的精度。为了得到表面换热系数与温度变化的关系,采用非线性估算法,编制计算程序,基于工件淬火过程的实测温度值,对工件在不同淬火介质中冷却过程的表面换热系数值随温度的变化进行了测算,得出了换热系数在冷却过程不同阶段的变化规律。     

双肋式微型气动阀的数值计算与实验

 针对现有微型三角阀效率低的问题,提出双肋式气动阀这一新型微阀,通过两级带圆弧过渡的收敛形肋条,在减小正向气流压力损失的同时,引导逆向气流分为3股后再呈“Y”形汇聚,产生强烈的相互撞击而抵消部分动能,从而减小逆向流量以提高效率。通过数值计算对双肋式气动阀的作用原理进行了分析与验证;加工了特征尺寸为1 mm的三角阀、梯形阀与双肋阀实验件,并设计了相应的实验方案,在微流体实验平台上进行了对比实验。结果表明双肋阀能大幅提高效率：对不可压流,双肋阀可将效率从普通阀的2%～3%提升至14%左右;对可压流,双肋阀能将效率从2%提升至约13%。     

交错肋结构形式对换热和流阻特性的影响试验研究

通过试验,研究了不同结构的交错肋对换热及流阻特性的影响。试验结果表明:努塞尔数和流阻系数,随着肋宽的增大而都增大,随着肋间距的增大而都减小,随着肋倾角的增大而都增大。综合换热效果为1.3~2.5。     

The Origin of Mercury’s Internal Magnetic Field

Mariner 10 measurements proved the existence of a large-scale internal magnetic field on Mercury. The observed field amplitude, however, is too weak to be compatible with typical convective planetary dynamos. The Lorentz force based on an extrapolation of Mariner 10 data to the dynamo region is 10⁻⁴ times smaller than the Coriolis force. This is at odds with the idea that planetary dynamos are thought to work in the so-called magnetostrophic regime, where Coriolis force and Lorentz force should be of comparable magnitude. Recent convective dynamo simulations reviewed here seem to resolve this caveat. We show that the available convective power indeed suffices to drive a magnetostrophic dynamo even when the heat flow though Mercury’s core–mantle boundary is subadiabatic, as suggested by thermal evolution models. Two possible causes are analyzed that could explain why the observations do not reflect a stronger internal field. First, toroidal magnetic fields can be strong but are confined to the conductive core, and second, the observations do not resolve potentially strong small-scale contributions. We review different dynamo simulations that promote either or both effects by (1) strongly driving convection, (2) assuming a particularly small inner core, or (3) assuming a very large inner core. These models still fall somewhat short of explaining the low amplitude of Mariner 10 observations, but the incorporation of an additional effect helps to reach this goal: The subadiabatic heat flow through Mercury’s core–mantle boundary may cause the outer part of the core to be stably stratified, which would largely exclude convective motions in this region. The magnetic field, which is small scale, strong, and very time dependent in the lower convective part of the core, must diffuse through the stagnant layer. Here, the electromagnetic skin effect filters out the more rapidly varying high-order contributions and mainly leaves behind the weaker and slower varying dipole and quadrupole components (Christensen in Nature 444:1056–1058, 2006). Messenger and BepiColombo data will allow us to discriminate between the various models in terms of the magnetic fields spatial structure, its degree of axisymmetry, and its secular variation.     

联合应用现代优化方法与S2流面计算进行多级涡轮的气动设计

本文联合应用S2流面正问题计算和多级局部优化设计对某三级涡轮进行多级气动优化设计。优化联合采用人工神经网络和遗传算法,流场计算采用全三维粘性流N-S方程求解,计算网格采用H-O-H型网格,即入口段、出口段采用H型网格,叶片区域采用O型网格。通过优化,总效率提高1.1%,总体性能提高,达到设计要求。     

二次流喷射对喷管流场性能的影响

采用有限体积法求解二维守恒型雷诺平均N-S方程,数值模拟了单膨胀斜面喷管内外流场,研究了二次流喷射对单膨胀斜面喷管非设计状态性能的影响,给出了性能随喷射流量、喷射总压和喷射角度的变化规律。计算结果表明,在喷管下斜板尾缘进行二次流喷射可以提高喷管非设计状态性能,喷射流量和喷射角度是影响喷管性能提高的主要因素,并存在最优的喷射流量和喷射角度,喷射总压对喷管性能影响较小。     

粉末燃料冲压发动机理论性能分析

研究粉末燃料冲压发动机的理论性能,采用编制的热力计算软件,分别对以硼粉、铝粉、镁粉为燃料的发动机性能进行了计算,分析了不同参数对发动机比冲的影响趋势,为进一步研究及发动机设计奠定了基础。通过与常规液体燃料冲压发动机及固体火箭冲压发动机进行比较,说明了粉末燃料冲压发动机在比冲及体积比冲方面的优势。鉴于金属粉末燃烧产物中凝相物质含量高的特点,研究了两相流损失对发动机性能的影响。     

湍流燃烧模型对氢燃料超燃室流场模拟的影响

采用化学平衡的假定概率密度函数(PDF)模型和火焰面模型计算了德国宇航研究中心的超燃室反应流,计算结果与有限速率反应模型的和实验的结果进行了对比.使用有限体积法离散Favre平均的N-S方程,湍流模型采用k-ε模型.研究表明:(1)有限速率反应模型在喷氢孔近场,化学平衡的假定PDF模型在喷氢孔远场不能准确捕捉流场的细致结构,而火焰面模型对全流场预测较好,后两种模型的计算时间较有限速率反应模型节省约38%;(2)超燃室内湍流和燃烧相互作用不可忽略,从预测精度和计算效率来看,火焰面模型有较好的工程应用前景.      

振动能量流的测量不确定度评定

介绍了管壁振动能量流的测试方法和不确定度来源,并进行了详细的分析和评定.     

多段翼型绕流的数值模拟研究

采用C—H型混合的结构化网格,选用Wilcox提出的k-ω模型求解可压的N-S方程,模拟了多段翼型的流场。结果表明：在4°和6°迎角下的非定常计算结果与试验结果的对比,计算结果与试验值吻合的较好。本文应用了亚迭代时间法,正确地描述了30P30N多段翼型前缘结构区域的流动特征和流动机理。