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.     

第2009卡林顿周太阳活动的初步分析

介绍了第 2 0 0 9卡林顿周大黑子群AR484,AR486和AR488产生的太阳活动以及这些太阳活动对地球空间环境造成的影响。依据对太阳活动的统计研究 ,简要分析了三个大黑子群活动的差异。分析结果指出 ,关注某一时期太阳活动的活动经度带以及太阳活动在某一半球的主次是解决太阳活动短期预报非常重要的思路     

Substorms in the inner plasma sheet

Thin Current Sheets (TCS) are regularly formed prior to substorm breakup, even in the near-Earth plasma sheet, as close as the geostationary orbit. A self-consistent kinetic theory describing the response of the plasma sheet to an electromagnetic perturbation is given. This perturbation corresponds to an external forcing, for instance caused by the solar wind (not an internal instability). The equilibrium of the configuration of this TCS in the presence of a time varying perturbation is shown to produce a strong parallel thermal anisotropy (T T) of energetic electrons and ions (E>50keV) as well as an enhanced diamagnetic current carried by low energy ions (E<50keV). Both currents tend to enhance the confinement of this current sheet near the magnetic equator. These results are compared with data gathered by GEOS-2 at the geostationary orbit, where the magnetic signatures of TCS, and parallel anisotropics are regularly observed prior to breakup. By ensuring quasi-neutrality everywhere we find, when low frequency electromagnetic perturbations are applied, that although the magnetic field line remains an equipotential to the lowest order in T_e/T_i, a field-aligned potential drop exists to the next order in (T_e/T_i). Thus the development of a TCS implies the formation of a field-aligned potential drop ( few hundred volts) to ensure the quasi-neutrality everywhere. For an earthward directed pressure gradient, a field-aligned electric field, directed towards the ionosphere, is obtained, on the western edge of the perturbation (i.e. western edge of the current sheet). Thus field aligned beams of electrons are expected to flow towards the equatorial region on the western edge of the current sheet. We study the stability of these electron beams and show that they are unstable to “High Frequency” (HF) waves. These “HF” waves are regularly observed at frequencies of the order of the proton gyrofrequency (f_H+) just before, or at breakup. The amplitude of these HF waves is so large that they can produce a strong pitch-angle diffusion of energetic ions and a spatial diffusion that leads to a reduction of the diamagnetic current. The signature of a fast ion diffusion is indeed regularly observed during the early breakup; it coincides with the sudden development of large amplitude transient fluctuations, ballooning modes, observed at much lower frequencies (fH+). These results suggest that the HF waves, generated by field-aligned electron beams, provide the dissipation which is necessary to destabilize low frequency (ballooning) modes.     

轴向充磁圆筒型永磁直线同步电机气隙磁场解析计算

介绍了一种基于许-克变换法的轴向充磁结构圆筒型永磁直线同步电机(TPMLSM)气隙磁场解析计算方法。首先采用许-克变换法计算出无齿槽时电机的气隙磁场;然后利用许-克变换法求取初级铁心开槽时的气隙相对比磁导函数,分析铁心开槽对气隙磁场的影响;最后通过无齿槽时的气隙磁场与有齿槽时的气隙磁场相对比磁导函数得到有齿槽时电机的气隙磁场分布。同时给出了该种充磁结构TPMLSM气隙磁场解析计算表达式,并以1台36/12极槽配合轴向充磁TPMLSM样机进行试验。试验结果证明空载气隙磁场的有限元分析值与解析值较吻合,空载电动势(EMF)计算值、试验测试值、有限元分析值一致。     

吸力面不同吹风比切向冷气喷射对跨声速涡轮叶栅气动性能的影响

为进一步探究跨声速涡轮中吸力面切向冷气喷射对叶栅气动性能及气膜冷却效果的影响,以跨声速涡轮叶栅作为研究对象,采用数值模拟方法,通过在叶片吸力面不同位置开设切向冷气喷射槽,进行不同吹风比下的冷气喷射,对跨声速气冷涡轮叶栅的总体性能以及流场细节进行了详细研究。研究结果表明,吸力面切向冷气喷射有利于减小跨声速涡轮叶栅激波损失,叶栅最大马赫数可减小0.104;切向冷气喷射槽位于尾缘内伸激波反射点上游,且吹风比处于0.75～1.00内时,叶栅能量损失最小;吹风比的增大有利于减小甚至消除冷气槽内分离泡,并能够减小唇部激波强度。     

基于地形匹配的高超声速飞行器初始定向偏差在线辨识方法

针对高超声速飞行器机动发射条件下自瞄准时间短、初始定向偏差大的问题，提出一种基于地形匹配的初始定向偏差在线辨识方法。以综合初始对准和姿态控制的惯性系统导航误差模型为分析基础，融合相邻两个地形匹配区两次地形匹配定位结果，建立了初始定向偏差在线辨识模型，并从惯性系统工具误差系数偏差和地形匹配定位误差两方面讨论了辨识模型的适应性。以美国高超声速飞行器CAV H为研究对象建立仿真环境，采用蒙特卡洛法检验初始定向偏差辨识效果。仿真结果表明，在地形匹配定位误差为173.88 m (3σ)情况下，初始定向剩余偏差平均值为8.42″，最大值为34.65″，能够有效提高惯性系统导航精度，并且有助于缩短发射准备时间、提高武器系统生存能力。     

超声速涡轮叶型全局气动优化设计

针对涡轮叶型全局优化设计计算时间长、样本空间大等难点提出一种可行的优化设计方法,该方法将控制叶型的17个参数作为优化变量,采用第二代多目标遗传算法进行全局自动寻优。基于此方法,搭建了涡轮叶型全局优化设计平台。利用此平台,分别采用轴向稠度固定和自由优化两种方式对超声速涡轮叶型进行了优化设计。数值计算结果表明,两组优化设计叶型在设计工况下总压损失系数比参考叶型分别低19.5%和10.0%,流道中的激波强度更弱,且在变工况条件下都具有较好的气动性能。深入分析流场与激波结构后发现,外尾激波相比于内尾激波对总损失的影响更大,通过减小气流膨胀转折角或内尾激波气流转折角能够有效削弱外尾激波强度。     

高速滚动轴承-转子系统的摩擦阻尼减振

为了抑制高速滚动轴承-转子系统在通过临界转速时的过大振动,本文采用了摩擦阻尼弹性支承结构.分析了该支承的减振机理和支承特性,设计了摩擦阻尼器,研究了其对转子系统不平衡响应的影响.结果表明,采用适当的机械结构,阻尼器的刚度因子和摩阻因子只与内环的锥角和接触面摩擦因数有关.通过改变这两个参数和外壳轴向刚度,可改变其刚度和阻尼特性.在转子系统支承中引入摩擦阻尼器能够降低支承刚度,从而降低系统的临界转速,避开工作转速.此外,还可增大支承阻尼,抑制临界振幅,减小系统的振动外传力.     

激波过弯道绕流流场(英文)

为了研究微波过弯道的传播，气动中心设计了微波过弯道的实验装置，它很容易拆卸并组成带10°发散的弯道、短形弯道和带各种角度的二元喷嘴。实验所得到的若干照片，对于研究激波反射、绕射与边界的相互作用和对数值模拟的验证是很有用的。