飞船返回舱高超声速气动特性的风洞实验分析

在返回舱再入过程中,高超声速配平升阻比是一个十分重要的参数。文章介绍球冠倒锥外形返回舱模型在φ0．5m高超声速风洞中气动力的测量结果,给出Ma=4．94、5．96、7．96,相应的Re=3×10^6、6×10^6、2×10^6（以最大横截面直径为特征长度）气流条件下,攻角从2°～-27°变化范围内返回舱的气动力特性,讨论重心位置纵移与横偏变化对配平升阻比和纵向稳定性的影响。     

EXPERIMENTAL STUDIES ON SWIRLING AND RECIRCULATING TWO-PHASE FLOW FIELD IN A COLD MODEL OF DUAL-INLET SUDDEN-EXPANSION COMBUSTOR

The axial and tangential velocities of gas and particle phases and particle concentration for turbulent swirling and recirculating gas-particle (simulating gas-droplet) flows in a cold model of a dual-inlet sudden-expansion combustor with partially tangential central tubes, proposed by the present authors, were measured by using a 2-D LDV system and a laser optic fiber system combined with a sampling probe. The results show that there are both gas and particle strongly reverse flows and swirling flows in the head part of the combustor. The velocity slip between gas and particle phases is remarkable. The particle concentration is higher near the wall and lower near the axis. There are two peaks in the concentration profiles near the inlet tubes. The above-obtained flow characteristics are favorable to ignition, flame stabilization and combustion. The results can also be used to validate the numerical modeling.     

扑动翼型的低雷诺数气动特性分析

通过求解引入拟压缩项的不可压Navier-Stokes方程,数值模拟了绕扑动翼型的低雷诺数非定常流动。针对厚度在4%-12%之间的NACA对称翼型,分析了翼型厚度等参数对扑动翼型气动特性的影响。在低雷诺数条件下,对于纯俯仰运动,随着翼型厚度的减小,平均阻力系数也变小。而对于纯沉浮运动,发现翼型厚度对气动特性的影响和俯仰运动有很大的差别,平均阻力系数随着翼型厚度的减小而变大。通过对沉浮运动一个周期流线图的分析,认为这是翼型前缘涡的影响造成的。由于前缘涡的影响,翼型厚度增加,平均压差阻力系数变小,甚至会出现负值。雷诺数的影响研究表明,随着雷诺数的增加,扑动翼型的阻力系数减小的趋势越缓慢。     

Local stability analysis of interface region of astrophysical viscous shear flows with a gradual velocity gradient

In this paper, we extend the stability analysis of cold sharp shear flows to warm astrophysical cases with, inevitable, gradual velocity gradient in the interface region in the presence of viscosity effect. Using linear perturbation theory as well as the local approximation method, the instability growth rate of the excited electromagnetic modes has been investigated for the relativistic and non-relativistic cases of solar wind interacting with interstellar plasma medium. Results show that astrophysical shear systems with a small velocity gradient in the transition region are more stable rather than larger ones. Moreover, dependent on the viscosity coefficient value, the viscosity effects could have a positive role on the instability growth rate of the system in some range of initial bulk velocity, while it plays a destructive role in other velocity ranges.     

碱金属引射下的高超声速尾流的数值模拟

高超声速化学非平衡尾流的分析与计算是空气动力学中的一个重要课题。本文采用二阶精度的中心差隐格式，求解了抛物化的Ｎ－Ｓ方程，得到了高空２０ＫＭ及６０ＫＭ非平衡尾流的数值解，研究了碱金属引射对尾流电子密度的影响。计算结果表明引射碱金属对尾流电子密度影响明显，尾流电子密度因此增加了１～３个量级。文中化学反应模型采用十组元模型，组元包括Ｏ２、Ｎ２、Ｏ、Ｎ、ＮＯ、ＮＯ＋、Ｏ－２、Ｎａ、Ｎ＋ａ以及ｅ－。     

高超声速飞行器表面气动热和粘性摩擦力计算

本文给出了高超声速飞行器表面摩阻和传热系数 (斯坦顿数 )的计算结果。采用两种方法平面切面法亦即二维边界层近似法和工程方法计算了飞行器高超声速绕流的粘性效应 ,并对两种方法的计算结果作了仔细的比较。由文可见 ,对于在稠密大气层内 ,沿轨道运行头速度恒定的高超声速有翼飞行器 ,能够用本文所采用的两种方法计算其表面摩阻和热载荷。此二法可成功地应用于绕复杂形状物体的流动参数计算。     

典型激波针减阻降热特性及流动机理

为研究激波针对超/高超声速钝头飞行器进行减阻降热的相关特性,采用数值模拟方法对6种典型激波针构型的流动特征开展系统研究。给出了激波针长度、来流马赫数对流动特征的影响规律,并对其形成机理进行了探讨。结果显示:马赫数较低时,头部有扰流物的5种激波针在回流区即将分裂时减阻率最大;马赫数较高时,减阻率在回流区分裂前后出现局部峰值,但最大减阻率将出现在回流区分裂后更长的激波针长度下。马赫数为3时,6种构型减阻率达最大时的相对长度在0.8~1.2之间,相比而言,球型、半球型和双锥型的减阻效果最好,最大减阻率为45%~50%;圆锥型最差,为20%~25%,明显低于头部有扰流物的构型。相同的激波针长度下,头部有扰流物构型的减阻率随马赫数增大而增大,圆锥型则相反。流场回流区、分离激波、弓形激波、局部膨胀流动等导致的压力分布变化是构型整体阻力变化的主要成因。      

高超声速飞行器纵向飞行稳定域与迟滞分析

针对滑翔式高超声速飞行器纵向失稳问题,基于连续算法和分岔理论,求解并分析了特征点单参数分岔图、平衡分支的稳定性和突变点,得出在大迎角飞行时存在较为严重的失稳现象;最后分析了多吸引点和迟滞效应现象.研究结果表明,滑翔式高超声速飞行器在大迎角飞行时存在严重失稳、多吸引域和复杂迟滞运动.此结果在实现飞行器稳定飞行和控制器设计方面具有很好的参考价值.     

国外高超声速技术计划回顾与展望

回顾了近年来国外高超声速技术发展计划，总结了这些国家开展的飞行演示试验及地面试验的最新进展。     

A new two-scale model for large eddy simulation of wall-bounded flows

A new hybrid approach to model high Reynolds number wall-bounded turbulent flows is developed based on coupling a two-level simulation (TLS) approach (Kemenov and Menon, 2006 [1], 2007 [2] in the inner region with conventional large eddy simulation (LES) away from the wall. This new approach is significantly different from previous near-wall approaches for LES. In this hybrid TLS–LES approach, a very fine small-scale (SS) mesh is embedded inside the coarse LES mesh. The SS equations capture fine-scale temporal and spatial variations in all three Cartesian directions for all three velocity components near the wall. The TLS–LES equations are derived using a new scale separation operator that allows a smooth transition between the two regions, with the equations in the transition region obtained by blending the TLS large-scale and LES equations. New terms in the hybrid region are identified. The TLS–LES approach is used to study the near-wall features in canonical turbulent channel flows for a range of Reynolds number using relatively coarse large-scale (LS) grids. Results show that the TLS–LES approach is able to capture the effect of both the LS and SS features in the wall region consistently for the range of simulated Reynolds number.