跨声速涡轮叶栅两点优化目标函数研究

针对跨声速涡轮叶栅单点优化方法难以获得整体工况性能提升、多点优化方法难以确定合理目标函数形式的问题，提出了两点优化的方法。为了节约优化时间成本，优化过程采用EIF （Equivalent inviscid flow） 模型进行数值模拟，通过添加惩罚函数保证叶栅满足设计流量和负荷要求，并采用叶栅效率线性平均的目标函数形式进行评价。选择两组跨声速涡轮叶栅进行优化设计，并利用CFD方法分析叶型变化对流场马赫数、激波和损失产生的影响。结果显示，所提出的优化设计方法在保证设计工况性能的同时，能够提升叶栅整体工况性能。通过流场分析，揭示了激波结构变化对不同工况损失影响的定性规律。综合全文研究后，给出了一种适用于跨声速涡轮叶栅两点优化设计的目标函数形式。     

高超声速双模块内转式进气道的流动特性研究-Part II 攻角影响

为了研究飞行攻角对高超声速双模块内转式进气道流动的影响,本文通过试验和仿真方法,获得了0°,4°和6°攻角条件下进气道模块内的流动结构。结果表明：在本文研究的攻角范围内,进气道均可起动,进气道压缩面侧的压力变化体现了基准流场的流动特性。在耦合作用下进气道模块间压缩面诱导的激波形态沿流向由弓形逐渐发展为钟形,并且在外压缩激波的扫掠影响下进气道的三个角区出现了强度不同的旋涡结构。进气道压缩面侧的角区旋涡随着攻角的增加而逐渐增强,而进气道出口截面上低能流区域随着攻角的增加而逐渐减小。低能流区域内的二次旋涡呈现不同的变化趋势,位于上半截面的旋涡随着攻角的增加其逐渐向上移动,而位于下半截面的旋涡位置基本保持不变。     

物体穿越斜激波干扰特性的数值研究

当物体以超声速穿越同向运动的斜激波时，它的飞行Mach数和攻角都会发生较大的变化。穿越过程中斜激波与物体脱体激波发生相互作用，形成复杂的激波干扰波系结构，基本的干扰形式为复合Mach反射结构。不同的穿越位置时，由于不同的来流条件，使物体上尾部凹坑内的流场和波系发生很大的变化，随着物体的穿越过程，当头部和凹坑下游壁面与翼面穿越激波时，阻力系数有两次剧烈的变化，法向力基本呈线性下降，压力中心先大幅度后移，物体逐渐穿过激波后又快速前移。因此穿越过程使物体加速，给物体的姿态带来很大的扰动。翼面穿过激波也造成阻力、法向力下降，压心后移。如果对有控制的飞行器，穿越激波时气动力特性和稳定性的急剧变化，将给控制系统带来很大的困难。     

激波和边界层相互作用区域局部烧蚀的理论计算方法

激波和边界层相互作用区域的局部烧蚀计算是极为复杂的非定常湍流分离流动条件下的烧蚀分析问题，本文将这一复杂的物理化学和气体动力学过程简化为二维前向台阶分离区的准定常烧蚀问题来处理，将偏微分的控制方程组简化为超越代数方程组，提供了一个有一定精度的理论分析方法，理论计算结果与实验数据相当吻合。     

计算尖锥迎面干扰的一种新方法

本文从运动气流的二维激波动力学方程组出发,提出了一种计算平面运动激波和尖锥头激波迎面干扰问题的新方法。该方法可以计算穿透激波的强度和形状,马赫反射时三波点的轨迹,马赫杆的强度和几何形状,以及锥面峰值压力的大小。计算结果与数值模拟、其它计算方法以及实验数据进行了比较,结果表明本方法不仅精度较高,而且保持了简捷,省机时的优点。     

Cylindrical and spherical dust-electron-acoustic shock waves due to dust charge fluctuation

Cylindrical and spherical dust-electron-acoustic (DEA) shock waves propagating in a dusty plasma (containing cold inertial electrons, hot Maxwellian electrons, stationary and streaming ions, and charge fluctuating stationary dust) are theoretically investigated by reductive perturbation method. It is shown that the effect of the dust charge fluctuation introduces some new features in the nonlinear propagation of the DEA waves, particularly the dust charge fluctuation provides a source of dissipation, and is responsible for the formation of the DEA shock structures. It is also found that the basic features of the DEA nonlinear structures are significantly modified by the non-planar (viz. cylindrical and spherical) geometry, and that the height of the cylindrical DEA shock structures are larger than that of the planar DEA shock structures, but smaller than that of the spherical ones. The implications of these results in laboratory dusty plasmas are briefly discussed.     

Diffusive shock acceleration at interplanetary perpendicular shock waves: Influence of the large scale structure of turbulence on the maximum particle energy

We calculate the maximum energy that a particle can obtain at perpendicular interplanetary shock waves by the mechanism of diffusive shock acceleration. The influence of the energy range spectral index of the two-dimensional modes of the interplanetary turbulence is explored. We show that changes in this parameter lead to energies that differ in at least one order of magnitude. Therefore, the large scale structure of the turbulence is a key input if the maximum particle energy is calculated.     

Anomalous particle transport in the heliosphere

The transport of energetic particles in the presence of magnetic turbulence can exhibit a variety of regimes different from the standard quasilinear diffusion. Here we discuss a number of solar and space problems where nonquasilinear diffusion is found, and then we illustrate anomalous transport regimes, for which the mean square deviation grows nonlinearly with time. In particular, we concentrate on superdiffusive regimes, and show what is the theoretical framework which is to be used to describe superdiffusion. We discuss the results of numerical simulations which show that superdiffusive and subdiffusive regimes are possible, and describe data analyses which allow to single out the superdiffusive transport from the observation of energetic particle profiles upstream of interplanetary shocks. The implications of superdiffusion on the efficiency of wave particle interactions are also discussed.     

Three dimensional investigation of the shock train structure in a convergent–divergent nozzle

Three-dimensional computational fluid dynamics analyses have been employed to study the compressible and turbulent flow of the shock train in a convergent–divergent nozzle. The primary goal is to determine the behavior, location, and number of shocks. In this context, full multi-grid initialization, Reynolds stress turbulence model (RSM), and the grid adaption techniques in the Fluent software are utilized under the 3D investigation. The results showed that RSM solution matches with the experimental data suitably. The effects of applying heat generation sources and changing inlet flow total temperature have been investigated. Our simulations showed that changes in the heat generation rate and total temperature of the intake flow influence on the starting point of shock, shock strength, minimum pressure, as well as the maximum flow Mach number.     

Mach reflection in steady supersonic flow considering wedge boundary-layer correction

Mach reflection in steady supersonic flow is an important phenomenon having received extensive studies, among which simplified theoretical models to predict the size of Mach stem and other flow structure are of particular interest. Past efforts for such models were based on inviscid assumption while in real cases the flow is viscous. Here in this paper we consider the influence of wedge boundary layer on the Mach stem height. This is done by including a simplified boundary layer model into a recently published inviscid model. In this viscous model, the wedge angle and the trailing edge height, which control the Mach stem height, are replaced by their equivalent ones accounting for the displacement effect of the wedge boundary layer, with the boundary layer assumed to be laminar or fully turbulent. This viscous model is shown to compare well with numerical results by computational fluid dynamics and gives a Mach stem height as function of the Reynolds number and Mach number. It is shown that due to the viscous effect, the Mach stem height is increased, through increasing the effective wedge angle.