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；     

轴向流中圆柱体的非线性动力学分析

通过引入流体摩擦力的二次阻尼项，推导出了轴向流中两端简支圆柱体的新的运动微分方程。对添加二次阻尼项的运动微分方程进行了无量纲化和Ritz-Galerkin离散。通过数值模拟，对两端铰支圆柱体的稳定性进行了系统的分析，并得出颤振发生的临界流速条件。     

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.     

二维射流的稳定性分析与流动控制

本文在绝对／对流不稳定性的理论框架下，对二维射流的稳定性进行了数值分析。研究表明射流流场各局部剖面是对流不稳定的，不会产生整体失稳，射流频率由流场中最大增长的不稳定频率确定。将一ＮＡＣＡ０１２翼型放置于射流势流核心区中，改变翼型的偏转角度θ，可使射流剪切层频率与翼型尾流频率发生共振，整个流场产生自激振荡，加强了射流与外界流场和混合，并使射流发生矢量偏转。     

冲压发动机燃烧室内低频燃烧不稳定试验

在高空亚燃冲压发动机研究中,燃烧不稳定是一个突出问题.为解决30km,Ma =4亚燃冲压发动机直连式试验中所出现的低频燃烧不稳定问题,分析了燃烧室的声学特性,得出了燃烧不稳定的主要特征是燃烧放热与一阶纵向声振模态相藕合.采取在燃烧室内增加后向台阶形成凹腔的方法,成功得到了较为稳定的燃烧.     

一种基于谱方法的三维热声不稳定模型

研究流体的流动参数,包括热源热释放的周向不均匀分布对热声不稳定现象的影响,将欧拉方程进行线化处理之后,对轴向和径向方向进行基于切比雪夫多项式的谱离散,周向方向则进行基于傅里叶多项式的谱离散,建立了一种三维热声不稳定数值模型.通过对圆柱管道共振频率以及声场的求解,进行了一系列算例的验证,证实了该方法的可靠性,并且通过热释...     

Transition study of 3D aerodynamic configures using improved transport equations modeling

As boundary layer transition plays an important role in aerodynamic drag prediction,the proposal and study of transition prediction methods simulating the complex flow phenomena are prerequisite for aerodynamic design. In this paper, with the application of the linear stability theory based on amplification factor transport transition equations on the two-equation shear stress transport(SST) eddy-viscosity model, a new method, the SST-N TS-N CF model, is yielded. The new amplification factor transport equation for the crossflow instability induced transition is proposed to add to the N TS equation proposed by Coder, which simulates Tollmien–Schlichting wave transition. The turbulent kinetic energy equation is modified by introducing a new source term that simulates the transition process without the intermittency factor equation. Finally, coupled with these two amplification factor transport equations and SST turbulence model, a four-equation transition turbulence model is built. Comparisons between predictions using the new model and wind-tunnel experiments of NACA64(2)A015, NLF(2)-0415 and ONERA-D infinite swept wing and ONERAM6 swept wing validate the predictive quality of the new SST-N_(TS)-N_(CF) model.     

反射激波作用下重气柱界面演化的PIV研究

在水平激波管中采用PIV方法研究了反射激波作用下SF6重气柱界面的发展演化。采用射流方法形成SF6无膜气柱界面,并以乙二醇作为示踪粒子。利用连续激光片光源结合高速摄影相机对流场进行显示,得到了反射激波作用下SF6气柱界面的发展过程。结果表明,入射激波的冲击会在界面上产生反向旋转的涡环结构,而反射激波的作用会在界面上产生与初始涡环旋转方向相反的次级涡环结构。此外,对反射激波作用后的流场图像进行PIV后处理,获得了流场连续的速度场和涡量场。获得的环量与已有的理论模型进行比较,取得了较好的一致性,也验证了本文实验方法的可行性。     

带加热偏流的声衬对热声不稳定性的控制方法

通过实验方法研究了热声不稳定性极其被动控制方法。搭建了水平放置的Rijke管热声不稳定性实验装置,采用电加热的热丝作为热源。实验中发现加热功率及加热丝前后空气的温度比对热声不稳定性的发声强度有着一定的影响。实验中尝试了采用背腔和穿孔板结构的声衬对热声不稳定性进行控制。其中背腔中可以通入偏流空气,且偏流空气的流量、温度均可以调节。实验发现:背腔中通入偏流空气可以增强对不稳定性的抑制效果,且随偏流速的增加，控制效果变好。此外,发现提高偏流空气的温度对提高声衬对热声不稳定性的控制效果作用不明显。