Stall flutter prediction based on multi-layer GRU neural network

The modeling of dynamic stall aerodynamics is essential to stall flutter, due to the flow separation in a large-amplitude pitching oscillation process. A newly neural network based Reduced Order Model (ROM) framework for predicting the aerodynamic forces of an airfoil undergoing large-amplitude pitching oscillation at various velocities is presented in this work. First, the dynamic stall aerodynamics is calculated by solving RANS equations and the transitional SST-γ model. Afterwards, the stall flutter bifurcation behavior is calculated by the above CFD solver coupled with structural dynamic equation. The critical flutter speed and limit-cycle oscillation amplitudes are consistent with those obtained by experiments. A newly multi-layer Gated Recurrent Unit (GRU) neural network based ROM is constructed to accelerate the calculation of aerodynamic forces. The training and validation process are carried out upon the unsteady aerodynamic data obtained by the proposed CFD method. The well-trained ROM is then coupled with the structure equation at a specific velocity, the Limit-Cycle Oscillation (LCO) of stall flutter under this flow condition is predicted precisely and more quickly. In order to predict both the critical flutter velocity and LCO amplitudes after bifurcation at different velocities, a new ROM with GRU neural network considering the variation of flow velocities is developed. The stall flutter results predicted by ROM agree well with the CFD ones at different velocities. Finally, a brief sensitivity analysis of two structural parameters of ROM is carried out. It infers the potential of the presented modeling method to depict the nonlinearity of dynamic stall and stall flutter phenomenon.     

基于逆间隙环节的飞机极限环振荡抑制方法

借鉴数学中的函数与反函数思想,由间隙环节的数学模型导出逆间隙环节。分析了飞机侧偏控制系统 中副翼、方向舵舵机间隙非线性特性所引起的极限环振荡,针对副翼、方向舵舵机的非线性特性设计了相应的逆间隙环节,把所设计的逆间隙环节引入侧偏控制系统。仿真结果表明,所设计的逆间隙环节能够显著地抑制侧偏控制系统中的极限环振荡。     

液体火箭发动机中频耦合振荡初步研究

为了研究常规液体火箭发动机研制中出现的中频流量型耦合振荡问题,对发动机耦合系统中各环节建立了满足声学分析的线性化频域模型.通过比较供应系统和燃烧室的幅频响应,并分析耦合系统的自由振荡复频率,以判断发动机的耦合稳定性.计算结果符合发动机试车规律,能够有效地反映该类型不稳定的特征.进一步讨论了燃烧时滞、喷注压降、管路长度和安装节流圈对系统耦合不稳定的影响规律,并揭示了该类型不稳定的机理.     

流量调节器管路系统自激振荡特性研究（液体火箭推进专刊）

流量调节器管路系统在小流量大压降工况下会出现低频自激振荡现象,为了深入认识自激振荡产生机理,结合某型自稳流型流量调节器及管路系统,基于流量调节器弹簧振子动力学模型开展数值仿真研究。数值仿真得出自激振荡频率为94 Hz,与发动机试验结果一致。自激振荡产生机理是流量调节器的液动力受滑阀窗口型面变化率影响对系统形成正反馈作用,流量调节器综合刚度小于零时系统失稳。分析了流量调节器结构参数对系统稳定性的影响作用,三角形滑阀节流口流通面积能够抑制管路系统自激振荡。结合某型流量调节器负载特性试验系统进行验证,得出随着流量调节器压降升高,管路系统稳定性变差,获得的幅频特性,稳定边界与试验结果一致。     

翼型纵向俯仰非定常气动力研究

飞行器飞行时受到的非定常气动力是飞行器设计以及机动飞行中须考虑的一个重要因素。采用CFD方法数值模拟了NACA0012翼型在马赫数从0.2~5.0范围变化时做强迫振荡的非定常流场。通过积分法计算了在不同马赫数时翼型的俯仰动导数。计算结果表明,迟滞效应随马赫数的增大先增大后减小,在跨声速区域迟滞效应达到最大;迟滞环的绕向在跨声速区域为顺时针方向;迟滞环顺时针绕向时,动导数大于零,模型动不稳定,逆时针绕向时,动导数小于零,模型动稳定;旋转角速度越大,翼型表面非定常气动效应越明显。     

直升机贴地飞行时的驾驶员诱发振荡研究

主要阐述直或机贴地飞行时的驾驶员诱发振荡问题，导出了贴地突防和迅速停止动作、地形跟踪时的“海豚”运动和贴地飞行时滑雪运动条件下诱发振荡时操纵位移和稳定裕度的计算公式，计算了Ｚ－８直长机的纵向试验结果，并进行了误差分析。计算结果表明，所研究的方法是可行的，可推广应用于各种直升机的闭环分析和计算。     

某型飞机空中飘摆故障分析及防护措施

分析某型飞机平尾助力器故障导致飞机在空中飞行时产生飘摆现象的原因,提出修理改进措施及维护对策。     

一种抑制电传系统PIO的非线性补偿方法

提出了一种不完全非线性补偿方法用来抑制电传系统飞行员诱发振荡,其补偿着眼点是电传系统内部的舵回路速率饱和。本文把新的补偿方法用于一个两回路的飞行控制系统中,其设计过程和仿真结果表明,该方法结构简单,可以有效抑制ＰＩＯ,而且不影响原有系统的正常工作,便于工程应用。     

三角形截面高柔结构横风向振动的风洞试验研究

本文介绍了正三角形截面高柔结构模型在均匀流场和湍流场中三种迎角下的横风向风振响应风洞试验结果,分析了三角形截面高柔结构的横风向涡激振动现象与驰振危险性,获得了一些数据和结论。     

Dependence of the 27-day variation of cosmic rays on the global magnetic field of the Sun

We show that the higher range of the heliolongitudinal asymmetry of the solar wind speed in the positive polarity period (A > 0) than in the negative polarity period (A < 0) is one of the important reasons of the larger amplitudes of the 27-day variation of the galactic cosmic ray (GCR) intensity in the period of 1995–1997 (A > 0) than in 1985–1987 (A < 0). Subsequently, different ranges of the heliolongitudinal asymmetry of the solar wind speed jointly with equally important corresponding drift effect are general causes of the polarity dependence of the amplitudes of the 27-day variation of the GCR intensity. At the same time, we show that the polarity dependence is feeble for the last unusual minimum epoch of solar activity 2007–2009 (A < 0); the amplitude of the 27-day variation of the GCR intensity shows only a tendency of the polarity dependence. We present a three dimensional (3-D) model of the 27-day variation of GCR based on the Parker’s transport equation. In the 3-D model is implemented a longitudinal variation of the solar wind speed reproducing in situ measurements and corresponding divergence-free interplanetary magnetic field (IMF) derived from the Maxwell’s equations. We show that results of the proposed 3-D modeling of the 27-day variation of GCR intensity for different polarities of the solar magnetic cycle are in good agreement with the neutron monitors experimental data. To reach a compatibility of the theoretical modeling with observations for the last minimum epoch of solar activity 2007–2009 (A < 0) a parallel diffusion coefficient was increased by ∼40%.