多电飞机电源系统的负载稳定性分析

阐述了恒功率负载的概念及其特性,介绍了电源系统中恒功率负载的工作原理,并对多电飞机电源系统的系统特性进行了分析。在此分析基础上,提出了解决负阻抗特性引起的飞机电源系统不稳定的方法,最后给出了保证系统稳定的条件。     

壁面的表面粗糙度引起的Stokes层亚临界不稳定性

用数值模拟的方法研究了二维壁面的表面粗糙度下Stokes层的非线性亚临界不稳定性问题.发现当粗糙度高度极小时,响应系数曲线与线性情况就会产生较大偏离.随着粗糙度高度的增加,扰动1阶谱会出现亚谐波的成分,粗糙度高度的进一步增加使扰动1阶谱进入混乱阶段,显示出亚临界失稳的过程.根据粗糙度高度与扰动1阶谱演化的特征关系,定义了临界粗糙度高度,并给出临界粗糙度高度与雷诺数的关系曲线.结果表明:临界粗糙度高度随着雷诺数增大而减小.雷诺数为300左右时,微米量级的粗糙度高度就可能引起Stokes层的亚临界失稳,发生转捩,由此也可以给出实验中观测到的转捩通常都发生在雷诺数为300附近的原因.      

文氏管出口张角对旋流杯流动不稳定性的影响

为探究旋流杯内流动不稳定现象,针对带不同出口张角文氏管的旋流杯冷态流场进行了大涡模拟,并结合PIV试验结果进行了验证。研究结果表明,文氏管出口张角对时均流场的影响主要在旋流杯内部区域,对下游恢复区域基本无影响;旋流杯瞬态流场中存在旋进涡核（PVC）和小涡旋结构,出口张角对PVC的运动频率和形态基本无影响,对小涡旋结构影响较大,相同Q值下,56°张角旋流杯方案的小涡旋结构更丰富;经本征正交分解方法（POD）分析,旋流杯的强脉动结构为PVC和小涡旋结构。56°张角旋流杯方案的小涡旋结构能量更强,脉动幅度较大,能更好地对燃油进行剪切破碎,有利于强化雾化效果。     

脉动燃烧机理和抑制的初步研究

研究了驱动压力力脉地脉动燃烧器冷态压力脉动特性的影响，还研究了驱动压力脉 温度脉动的相位差对燃烧器系统的压力脉动特性的影响。频谱图表明，ｆ＝（１＋ｍ）ｆｄ（有时ｆ（１／２＋ｍ）ｆｄ处，都再现压力脉动的峰值），ｆ＝（１＋ｍ）ｆｄ＝（１＋ｎ）ｆ０时压力脉动的幅值大于ｆ＝（１＋ｍ）ｆｄ＝（１／２＋ｎ）ｆ０或ｆ＝（１／２＋ｍ）ｆｄ＝（１／２＋ｎ）ｆ０的幅值，当驱动压力脉动和温度脉动频率相同相位相近时，脉动     

电离层中SEE现象的静电粒子模拟

利用网格粒子云（PIC）模型。在一定条件下，对电离层加热实验中静电波的激发和参量不稳定性的产生，作一维静电粒子模拟，模拟结果表明，SEE的特征与加热泵波频率ω0和电子回旋频率nωce之间的比值有关。入射泵波的电场与地磁场之间的夹角也是影响SEE的一个因素。     

Non-linear diffusion of cosmic rays

The propagation of cosmic rays in the interstellar medium after their release from the sources – supernova remnants – can be attended by the development of streaming instability. The instability creates MHD turbulence that changes the conditions of particle transport and leads to a non-linear diffusion of cosmic rays. We present a self-similar solution of the equation of non-linear diffusion for particles ejected from a SNR and discuss how obtained results may change the physical picture of cosmic ray propagation in the Galaxy.     

后掠平板横流不稳定性

本文研究了无限后掠平板三维边界层的横流不稳定性，证明行进波和定常波几平同时失稳，且行进波比定常波更不稳定；     

Non-Linear Growth of Trapped Particle Modes in Linearly Stable, Current-Carrying Plasmas – A Fundamental Process in Plasma Turbulence and Anomalous Transport

The two-stream instability as a fundamental process in a current-carrying plasma is reconsidered. Its well-established linear version, based on kinetic Landau theory, predicts a threshold for the drift velocity between both species below which the plasma should be stable. We report on simulations which, however, show that a plasma as a non-linearly responding medium can be destabilized well below this threshold. Responsible for this unexpected behaviour are coherent, electrostatic, trapped particle structures such as phase space vortices or holes which can grow non-linearly out of thermal noise receiving their energy from the net imbalance of loss of electron kinetic energy and gain of ion kinetic energy. The birth of predominantly zero-energy holes is shown numerically being associated with initial, non-topological fluctuations. The latter are not subject to Landau damping, as they lie outside the realm of linear wave theory. For a pair plasma a typical scenario is presented, which encompasses several regimes such as non-linear growth of multiple holes, saturation and fully developed structural turbulence as well as an asymptotic approach to a new collisionless equilibrium. During the transient, structural state the plasma transport appears to be highly anomalous.