激光冲击残余应力场的有限元分析

建立模拟激光冲击残余应力场的非线性弹塑性有限元模型,预测AISI 304奥氏体不锈钢厚、薄靶材经激光冲击后表面以及内部的残余应力场分布.模拟过程中,考虑材料高应变率(106s-1)下的力学性能和激光诱导冲击波的精确加载,分析激光功率密度、激光光斑尺寸、激光脉宽、激光冲击次数、激光单面与双面冲击等激光冲击参数以及初始残余应力等因素对不锈钢靶材残余应力分布的影响.数值模拟结果与X射线衍射法测量值吻合较好.在有初始残余拉应力(250MPa)存在的情况下,激光冲击仍能使304奥氏体不锈钢靶材形成残余压应力层,说明激光冲击工艺可提高奥氏体不锈钢焊接构件的抗应力腐蚀开裂能力.     

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.     

电动汽车牵引用水冷异步电机耦合场分析

基于Ansys多物理场仿真分析平台,对1台车用异步电机进行多物理场耦合分析。仿真电机连续运行在额定工况和峰值工况下的温升和热应力,对电机各部分温度场分布进行深入分析,预测电机峰值工况的最长允许时间。通过热-结构的有限元仿真分析电机内部结构的热应力分布,深入分析转子导条端部与端环焊接位置和机壳与铁心过盈配合面的热应力,校核转子导条端部是否存在开焊的风险,并通过热仿真和应力分析计算机壳与铁心在最高温升工况下不发生滑移或涨开的过盈配合量取值。     

风电及高压电机用绝缘浸渍漆选型试验研究

选取国内常用的两种树脂与环氧酸酐浸渍树脂作对比测试。通过对树脂常规性能及浸渍模拟线圈电性能测试,得出结论:1号树脂具有较好的储存稳定性,电性能与环氧酸酐相当,可作为环氧酸酐的替代品。     

利用定子槽口宽度削弱永磁电机电磁噪声研究

着重研究了永磁电机定子槽口宽度对电磁噪声的影响。通过电磁力解析计算得出电磁力与定子槽口宽度的计算关系。利用Ansoft软件对1台电动汽车用永磁电机进行电磁场计算,求解改变定子槽口宽度对电磁力波的影响,并用ANSYS软件对该永磁电机进行不同定子槽口宽度的2D声场计算。进行了试验验证,仿真计算与试验结果基本一致,可为该类电机削弱噪声设计计算提供参考。     

回流燃烧室流动特性试验

为了揭示有/无燃烧状态下燃烧室热态和冷态流场的特征和流动特性,针对某型回流燃烧室单头部试验件,使用粒子图像测速仪（PIV）,测量燃烧室燃烧状态下不同截面处的热态流场,以及没有燃烧状态下不同截面处的冷态流场,探讨不同总压损失系数对回流燃烧室热态/冷态流场特征及流动特性的影响。研究表明:随着总压损失系数的增大,冷态条件下各截面流场结构基本保持不变,如射流孔穿透深度、射流角度、回流区位置及大小、流线等基本保持一致,但是各位置点速度大小逐渐增大。热态条件下各截面流场随着总压损失系数增大,流场结构也基本保持不变;相同总压损失系数时,热态流场与冷态流场存在差异,燃油喷射与气流的相对运动将会对燃烧室头部的流场结构造成影响,速度较冷态流动时略微增大。      

便携式充电设备检测系统的研究与设计

为了便于充电设备现场检测工作,设计了一种便携式直流充电设备现场检测系统。该系统功能具有完善的测试功能,能够方便的对直流充电设备进行检验测试,完全满足直流充电设备运行检测的需求。该系统具有小型化、便携化的优点,有利于提高现场检测效率,保证了充电设备运行的安全性及稳定性。     

开裂式方向舵在变前掠翼布局中的操纵性能研究

 针对变前掠翼(VFSW)无尾布局的横航向操纵,设计了开裂式方向舵(SR)操纵面,采用Navier-Stokes控制方程的有限体积离散方法以及剪切应力输运(SST)湍流模型,计算了变前掠翼中平直翼和典型的前掠翼布局开裂式方向舵的操纵性能,并对其操纵效率进行了比较,分析了其流场形态。计算结果表明:右侧开裂式方向舵打开后,平直翼时迎角对偏航力矩的影响较小,而舵偏量对偏航影响显著,利于偏航;前掠翼的偏航力矩随迎角的增加有所波动,但在小迎角时较为稳定,偏航作用随舵偏量增加而增强;右侧滑对滚转作用强于左侧滑,偏航作用低于左侧滑。经比较,平直翼的偏航作用明显强于前掠翼,平直翼和前掠翼的滚转和偏航作用均具有耦合性,但平直翼的耦合效应弱于前掠翼。     

复杂旋翼流场的耦合欧拉-拉格朗日数值方法

针对影响旋翼流场求解精度的关键因素“桨叶复杂近体流动”和“尾迹涡畸变”,结合计算流体力学(CFD)方法和黏性涡方法,发展了一套适合于复杂旋翼涡流场分析的耦合欧拉-拉格朗日数值方法:为捕捉桨尖三维效应、激波等细节流场特征,在桨叶近体区域采用CFD方法对其进行求解;针对高雷诺数旋翼流场中桨尖涡的紧凑结构特点,引入黏性涡方法建立了高分辨率的尾迹求解模型;两计算域间的信息交换采用了集中涡源法和边界修正法.应用所建立的计算方法,以旋翼CFD标准验证试验(Caradonna-Tung旋翼)为算例,对尾迹影响明显的悬停状态进行了数值模拟,通过对比耦合边界处流场特征及桨叶表面压力系数分布,验证了方法的有效性.此外,还从旋翼尾迹捕捉精度、涡量耗散特征及计算时间等方面对不同计算方法进行了对比分析,结果表明耦合方法可充分发挥CFD和黏性涡方法各自的优点,在旋翼流场数值模拟方面具有独特的优势.     

跨声速压气机转子叶尖非定常流场数值研究

采用时间精确求解方法对某高负荷跨声速轴流压气机转子在98%设计转速下的叶尖非定常流场进行了数值研究.结果显示,激波自身振荡不明显,叶尖区域流动的非定常性主要来源于叶尖泄漏涡的破碎及其与激波之间的相互干涉.对比设计状态与失速状态下叶尖泄漏涡的特点发现:在近失速点时,叶尖区域间歇性出现前缘溢流.分析表明:叶尖泄漏涡在激波后破碎是造成堵塞的主要原因,也是造成spike型失速初始扰动的原因.