部分充液悬臂转子在不稳定区的动力特性

 描述了试验中部分充液转子系统在失稳过程中的动力特性,注意了转子在不稳定区的涡动频率和方向,流体表面的状态与转子失稳之间的关系;研究了充液量对转子的涡动频率和不稳定区的影响。报道了部分充液转子系统在失稳过程中的一些重要现象,为深入研究部分充液转子系统失稳机理提供了实验依据。     

优化与人机交互设计方法及其在结构设计中的应用

 对于复杂的工程结构设计,除了要满足各种力学条件之外,往往还有许多制造与使用方面的要求,由专家的经验来判断和处理往往更为合理。因此,采用优化与人机交互相结合的设计方法,可以取长补短而获得更为合理和实用的结果。     

用粘流－无粘流相互作用方法计算翼型的分离和失速

本文用势流－边界层相互作用方法计算低速翼型的分离和失速。势流用对称面元法。边界层用改进的滞后掺混法，考虑了高阶项影响，适用于计算分离。文中对粘流－无粘流耦合方法作了改进。改进的半反－局部联立耦合方法，考虑了相邻点之间的作用，收敛性较好。计算了ＮＡＣＡ４４１２翼型在不同迎角下的压力分布和气动力。计算结果与实验符合良好。算例表明，翼型高升力状态计算必须包括尾流的作用，也应当对势流计算压力与实际压力之间的差别进行修正。     

A new fatigue life prediction model considering the creep-fatigue interaction effect based on the Walker total strain equation

The performance of high-temperature components of aero-engines under the Creep-Fatigue Interaction (CFI) behavior gets more attention recently. In this research, the creep-fatigue tests of two superalloys of Powder Metallurgy (PM) FGH96 and direct aging GH4169 were performed at 650 °C with different types of dwell, and the fracture morphology of FGH96 specimens was observed by Scanning Electron Microscopy (SEM) to analyze the creep-fatigue fracture feature and crack initiation. Additionally, according to phenomenology, the effect of dwell was introduced to develop a new uniaxial fatigue life prediction model based on the total strain equation, which has capability to take dwell time and load ratio into account together. The equations were utilized to model the test data of PM FGH96 and GH4169, together with data of another superalloy PM FGH95 conducted previously. A prominent prediction ability of the model in creep-fatigue life prediction of different superalloys has been manifested. Most data points of test data and estimated data are located within two times scatter band, which is ideal in engineering.     

热斑对涡轮级转静干涉噪声影响数值研究

利用结合相位延迟方法的求解器,对进口有热斑存在的某高压涡轮级流场进行三维非定常计算,然后利用模态匹配方法在涡轮转子下游管道中提取出转静干涉离散噪声信息.通过与进口无热斑存在算例比较表明:在一倍叶片通过频率下,向下游传播的转静干涉离散噪声总声功率级增加了约5.9dB;在二倍叶片通过频率下增加了约11.6dB.      

Analysis of blade vibration response induced by rotating stall in axial compressor

An experimental and numerical study was conducted to investigate the forced response of blade vibration induced by rotating stall in a low speed axial compressor. Measurements have been made of the transient stalling process in a low speed axial compressor stage. The CFD study was performed using solution of 3-dimensional Navier-Stokes equations, coupled with structure finite element models for the blades to identify modal shapes and structural deformations simultaneously. Interactions between fluid and structure were managed in a coupled manner, based on the interface information exchange until convergence in each time step. Based on the rotating stall measurement data obtained from a low speed axial compressor, the blade aeroelastic response induced by the rotating stall flow field was analyzed to study the vibration characteristics and the correlation between the phenomena. With this approach,good agreement between the numerical results and the experimental data was observed. The flow phenomena were well captured, and the results indicate that the rotating field stall plays a significant role in the blade vibration and stress affected by the flow excitation.      

凹腔前缘角对超声速燃烧室性能的影响

针对带有不同前缘角的凹腔内流动和燃烧过程,分别在冷态和燃烧条件下探讨了前缘角对凹腔内流动损失及阻力特性的影响.研究表明:在壁面垂直喷射的喷口上游和凹腔内部均会形成低速、高温回流区,有利于点火及火焰稳定,燃烧反压通过边界层的亚声速区域上传,形成激波/边界层干扰结构.减小前缘角,可使剪切层分离位置提前,更偏向凹腔内部,导致凹腔后壁面再附激波增强,进而增大了总压损失,降低了总压恢复系数;亦可导致凹腔前、后壁面压差阻力增大,阻力系数上升.进一步认识了凹腔内部流场及稳焰增混机理,进而为优化凹腔结构设计提供依据.      

Planetary wave coupling of the atmosphere–ionosphere system during the Northern winter of 2008/2009

This paper presents the global spatial (latitude and altitude) structure and temporal variability of the ∼23-day ionospheric zonally symmetric (s = 0) planetary wave (PW) seen in the Northern winter of 2008/2009 (October 2008–March 2009). It is shown that these ∼23-day ionospheric oscillations are forced from PWs propagating from below. The COSMIC ionospheric parameters f_oF2 and h_mF2 and electron density at fixed altitudes and the SABER temperatures were utilized in order to define the waves which are present simultaneously in the atmosphere and ionosphere. The long-period PWs from the two data sets have been extracted through the same data analysis method. The similarity between the lower thermospheric ∼23-day (s = 0) temperature PW and its ionospheric electron density response provides valuable and strong experimental evidence for confirming the paradigm of atmosphere–ionosphere coupling.     

Acceleration of energetic particles by whistler waves in active space experiment with charged particle beams injection

In this paper the investigation of wave-particle interaction during simultaneous injection of electron and xenon ion beams from the satellite Intercosmos-25 (IK-25) carried out using the data of the double satellite system with subsatellite Magion-3 (APEX). Results of active space experiment devoted to the beam-plasma instability are partially presented in the paper Baranets et al. (2007). A specific feature of the experiment carried out in orbits 201, 202 was that charged particle flows were injected in the same direction along the magnetic field lines B₀ so the oblique beam-into-beam injection have been produced. Results of the beam-plasma interaction for this configuration were registered by scientific instruments mounted on the station IK-25 and Magion-3 subsatellite. Main attention is paid to study the electromagnetic and longitudinal waves excitation in different frequency ranges and the energetic electron fluxes disturbed due to wave-particle interaction with whistler waves. The whistler wave excitation on the 1st electron cyclotron harmonic via normal Doppler effect during electron beam injection in ionospheric plasma are considered.     

利用多卫星观测CIR事件演变的统计分析

根据2007-2009年STEREO-BEHIND (STB)和ACE卫星的行星际磁场和太阳风数据, 基于冕洞高速流从太阳向外匀速径向传输假设, 讨论了随着STB和ACE卫星与太阳之间的夹角从0°增大至70°时, 冕洞发出的高速太阳风形成的相互作用区(CIR)依次扫过STB和ACE卫星的时间差特性, 并统计分析了两颗卫星观测到的CIR参数的变化特征. 结果显示, 可以利用STB对CIR事件的观测来预测这个CIR事件到达ACE的理论时间, 时间误差均值和最大值分别为0.217d和0.952d, 时间误差的产生与STB和ACE卫星观测到的CIR速度大小的不同有关, 用速度差异矫正后, 时间误差的平均值和最大值可分别减小为0.194d 和0.489d; STB和ACE卫星观测的CIR事件太阳风速度最大值的线性相关系数达到了0.84, STB和ACE卫星观测到的CIR事件对特征物理量中速度、质子温度的变化最小, 而质子密度及总压力的变化最大. 分析结果表明, STB和ACE卫星观测到的CIR事件有很强的相似性, STB卫星的CIR观测可以作为ACE卫星观测CIR事件特征的参考, 从而为地球空间环境扰动预报提供依据.