更替某型飞机电压限定器的研究

文章在介绍某型电压限定器工作原理的基础上,阐述了利用集成电路技术和自动控制技术进行该型电压限定器国产化研制的方法,给出了电压限定器探测及延时电路、均衡控制电路、防止误动作保护电路的详细设计方案,解决了激磁控制、均衡控制、故障鉴别等国产化研制过程中遇到的问题,保证了新研制产品与原有进口产品的可互换使用,提高了设备的工作可靠性。     

Nonlinear Dynamics Behaviors of a Rotor Roller Bearing System with Radial Clearances and Waviness Considered

A rotor system supported by roller beatings displays very complicated nonlinear behaviors due to nonlinear Hertzian contact forces, radial clearances and bearing waviness. This paper presents nonlinear bearing forces of a roller bearing under four-dimensional loads and establishes 4-DOF dynamics equations of a rotor roller bearing system. The methods of Newmark-β and of Newton-Laphson are used to solve the nonlinear equations. The dynamics behaviors of a rigid rotor system are studied through the bifurcation, the Poincar è maps, the spectrum diagrams and the axis orbit of responses of the system. The results show that the system is liable to undergo instability caused by the quasi-periodic bifurcation, the periodic-doubling bifurcation and chaos routes as the rotational speed increases. Clearances, outer race waviness, inner race waviness, roller waviness, damping, radial forces and unbalanced forces-all these bring a significant influence to bear on the system stability. As the clearance increases, the dynamics behaviors become complicated with the number and the scale of instable regions becoming larger. The vibration frequencies induced by the roller bearing waviness and the orders of the waviness might cause severe vibrations. The system is able to eliminate non-periodic vibration by reasonable choice and optimization of the parameters.     

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.     

基于感测线圈和KPCA的电机轴承故障检测

在电机定子中嵌入感测线圈并结合核主元分析(KPCA)进行电机轴承的故障检测。8只线圈分别嵌入电机定子的前端和后端,通过分时复用形成6组反应电机状态的差动信号。针对6组感测信号与电机状态间的非线性特征,采用KPCA进行多变量分析。着重介绍分析了KPCA故障检测的算法、监测指标和步骤。最后,用机车变压器油泵电机为对象开展了试验研究,验证了所提电机轴承故障监测方法的有效性和正确性。     

高转矩密度磁力齿轮的拓扑结构设计与性能比较

永磁行星齿轮和同轴永磁齿轮是两类具有不同拓扑结构和运行原理的磁力齿轮,采用定量设计比较法设计了具有相同有效体积和永磁体用量的上述两类磁齿轮,并通过有限元分析法对二者的转矩传递性能进行比较研究。研究结果表明,永磁行星齿轮较同轴永磁齿轮有更高的转矩密度和更低的转矩脉动。此外,由于永磁行星齿轮具有更加灵活的运行模式,并且能实现功率分流,使其在混合动力汽车领域有很好的应用前景。加工了一台永磁行星齿轮样机,并搭建试验平台进行了相关的试验,结果表明了该拓扑结构的有效性。     

水冷电机设计特点分析

水冷电机应用广泛,其设计也有自己的特点。针对水冷电机中机壳水冷结构的两种水路分布方式,即折返型和螺旋型,介绍了水路结构的优缺点和水路设计涉及参数的计算方法。考虑水冷机壳承压问题,给出了机壳内外筒壁强度计算公式。研究内容可为水冷电机的设计提供参考。     

轴流压气机插板式进气畸变数值仿真

以航空发动机稳定性评价体系中常用的插板实验为背景,分别进行低速、高亚声速、跨声速轴流压气机与插板畸变发生器的耦合数值仿真,研究插板畸变条件下压气机的流场特性以及不同类型压气机在插板畸变影响下的失速起始机制。研究发现:转子进口截面的周向流动是影响低速压气机稳定边界的主要因素;插板角涡对转子叶顶泄漏涡的扰动是影响高亚声速压气机稳定边界的重要原因;畸变气流影响下的叶片通道内激波强度和位置的变化是影响跨声速压气机稳定边界的关键因素。      

脉冲爆震载荷作用下转子系统动力学特性

针对脉冲爆震涡轮发动机(PDTE)气动载荷具有周期性、非定常的特点,应用有限元法建立了PDTE转子系统动力学特性计算模型。在验证计算模型准确性的基础上,研究了周期性、非定常轴向力和扭矩对转子系统动力学特性的影响。研究结果表明:与传统燃气涡轮发动机相比,PDTE转子系统同时存在弯曲振动、轴向振动和扭转振动。脉冲爆震燃烧室的气动载荷会改变转子系统的弯曲刚度,但对气动载荷合理设计后,其对弯曲振动的影响较小。周期性、非定常轴向力引起转子系统轴向振动,且轴向振动特性主要受零频和1阶轴向共振频率处响应的影响。PDTE工作时滚珠轴承的轴向支反力会不断变向,在设计滚珠轴承时应予以考虑。周期性、非定常扭矩引起转子系统扭转振动,1阶扭转共振频率分量在扭转振动响应中占优。      

模块化永磁直线游标电机等效磁网络及漏磁分析

在模块化永磁直线游标电机的初始设计及优化设计中,使用有限元方法(FEM)计算漏磁系数时需要耗费大量的建模和计算时间。针对这一问题,建立该种电机的等效磁网络模型,在建模期间,考虑气隙中的边缘效应,并计算永磁体组与定子齿在不同相对位置时的等效磁导,得到该种电机在一个周期内不同相对位置时的漏磁磁导和漏磁系数的数学解析表达式。采用FEM验证了该数学解析表达式的准确性。研究结果为模块化永磁直线游标电机的设计提供了理论依据。     

三支点柔性转子系统支承不同心激励特征及振动响应分析

针对航空发动机三支点柔性转子系统的支承不同心问题,充分考虑转子结构特征和载荷特征,首次将当量刚度引入多支点柔性转子不同心问题的动力学分析,定量描述转子系统各支承间不同心度带来的转子轴段刚度非线性,并提出了多跨度柔性转子系统支承不同心激励的数学描述,建立了不同心激励下多跨度柔性转子系统的力学模型。基于Lagrange能量法,给出了转子系统动力学方程的求解方法,研究得到了支承不同心转子系统的动力响应特征。结果表明:支承不同心不仅引起转子过渡轴的刚度非线性,产生2倍频激励,还会给转子系统带来附加不平衡激励;对于三支点柔性转子系统而言,2倍频分量同样是支承不同心下转子系统振动响应的典型特征之一。转子系统2倍频分量随不同心量的增加而迅速增加,而1倍频分量基本保持不变。同时转子振动响应呈现"缓增速降"趋势,且随非线性刚度、不平衡量的增大愈加明显。