涡升力乘波体发展研究综述

乘波飞行器在高超声速具有良好的气动性能,但偏离设计状态,气动性能则难以保持。为在宽速域范围能一直维持较好的气动性能,研究人员利用定平面形状乘波设计的优势,提出“涡升力”乘波设计。本文将涡升力乘波体的设计方法归纳为基于吻切理论的定前缘型线法、基于激波装配法的波导体法和基于给定激波面的投影法三大类,综述了涡升力乘波体在宽速域气动特性的相关研究进展,并对涡升力乘波体的后续研究提出建议。     

内并联式TBCC进气道模态转换过程流动特性分析

针对组合动力(TBCC)进气道模态转换过程中出现的非定常气动现象,采用稳态/非稳态数值模拟方法对相关流动特性及其影响因素与流动机理开展了研究。结果表明：由涡轮发动机工作状态向冲压发动机工作模态转换过程中,进气道内出现结尾激波沿流向前后振荡现象,振荡频率约为130Hz;当冲压流道反压引起的激波未前传至模态转换分流板前时,冲压发动机工作状态对结尾激波振荡不产生影响。在相同的发动机工作状态下,随着模态转换速度的增加,结尾激波振荡频率逐渐增大。文中研究的进气道内结尾激波振荡现象可通过亚声速管道内波的传播理论进行解释和分析。     

Height of shock formation in the solar corona inferred from observations of type II radio bursts and coronal mass ejections

Employing coronagraphic and EUV observations close to the solar surface made by the Solar Terrestrial Relations Observatory (STEREO) mission, we determined the heliocentric distance of coronal mass ejections (CMEs) at the starting time of associated metric type II bursts. We used the wave diameter and leading edge methods and measured the CME heights for a set of 32 metric type II bursts from solar cycle 24. We minimized the projection effects by making the measurements from a view that is roughly orthogonal to the direction of the ejection. We also chose image frames close to the onset times of the type II bursts, so no extrapolation was necessary. We found that the CMEs were located in the heliocentric distance range from 1.20 to 1.93 solar radii (Rs), with mean and median values of 1.43 and 1.38 Rs, respectively. We conclusively find that the shock formation can occur at heights substantially below 1.5 Rs. In a few cases, the CME height at type II onset was close to 2 Rs. In these cases, the starting frequency of the type II bursts was very low, in the range 25–40 MHz, which confirms that the shock can also form at larger heights. The starting frequencies of metric type II bursts have a weak correlation with the measured CME/shock heights and are consistent with the rapid decline of density with height in the inner corona.     

出口封闭的冲压发动机进气道激波振荡现象

采用计算流体力学和风洞试验两种手段,对冲压发动机出口封闭的多种超声速进气道内通道气流振荡现象进行了研究。结果表明,在一定的超声速范围内,封闭的进气道内通道发生了较强气流振荡现象,振荡频率、幅值和内通道长度、飞行马赫数有关,该振荡现象是一种自激振荡现象。利用亥姆霍兹共振器频率公式可以对封闭的进气道内通道振荡频率进行预估,并对其归纳出一种修正方法,可以结合模型试验结果对进气道和燃烧室内流振荡频率和幅值进行分析,为飞行试验提供预估和参考。     

Calculation of an unsteady jet flow around the plate cascade

In the framework of the general theory for unsteady weakly disturbed fluid flows with free boundaries, a problem is solved to calculate a jet flow around the cascade of plates executing the harmonic oscillations. We developed a program that enables us for the first time to carry out systematic calculations of flow characteristics depending on arbitrary values of determining parameters.     

Possible physical properties of the flow in the vicinity of the heliopause

An interface between the fully ionized hydrogen plasma of the solar wind (SW) and the partially ionized hydrogen gas flow of the local interstellar medium (LISM) is formed as a region where there is a strong interaction between these two flows. The interface is bounded by the solar wind termination shock (TS) and the LISM bow shock (BS) and is separated on two regions by the heliopause (HP) separating the solar wind and charged component of the LISM (plasma component below). The BS is formed due to the deceleration of the supersonic LISM flow relative to the solar system. Regions of the interface between the TS and HP and between the HP and BS were in literature named as the inner and outer heliosheaths, respectively. An investigation of the structure and physical properties of the heliosheath is at present especially interested due to the fact that Voyager-1 and Voyager-2 have crossed the TS in December 2004 (Burlaga, L.F., Ness, N.F., Acuna, M.Y., et al. Crossing the termination shock into the the heliosheath. Magnetic fields. Science 309, 2027–2029, 2005; Fisk, L.A. Journey into the unknown beyond. Science 309, 2016–2017, 2005; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Voyager 1 in the foreshock, termination shock and heliosheath. Science 309, 2020–2024, 2005; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. Voyager 1 explores the termination shock region and the heliosheath beyond. Science 309, 2017–2020, 2005) and in September 2007 (Jokipii, J.R. A shock for Voyager 2. Nature 454, 38–39, 2008; Gurnett, D.A., Kurth, W.S. Intense plasma waves at and near the solar wind termination shock. Nature 454, 78–80, 2008. doi: 10.1038/nature07023; Wang, L., Lin, R.P., Larson, D.E., Luhmann, J.G. Domination of heliosheath pressure by shock-accelerated pickup ions from observations of neutral atoms. Nature 454, 81–83, 2008. doi: 10.1038/nature07068.14; Burlaga, L.F., Ness, N.F., Acuna, M.H., et al. Magnetic fields at the solar wind termination shock. Nature 454, 75–77, 2008. doi: 10.1038/nature07029; Richardson, J.D., Kasper, J.C., Wang, C., et al. Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock. Nature 454, 63–66, 2008. doi: 10.1038/nature07024; Stone, E.C., Cummings, A.C., McDonald, F.B., et al. An asymmetric solar wind termination shock. Nature 454, 71–74, 2008. doi: 10.1038/nature07022; Decker, R.B., Krimigis, S.M., Roelof, E.C., et al. Mediation of the solar wind termination shock by non-thermal ions. Nature 454, 67–70, 2008. doi: 10.1038/nature 07030), respectively, and entered to the inner heliosheath.     

采用伪速度冲击响应谱评估蜂窝夹层板破坏边界

采用伪速度冲击响应谱(PVSRS)对航天器蜂窝夹层结构进行了冲击破坏边界评估。目前航天领域常用的冲击响应谱(SRS)是绝对加速度谱(AASRS)，相较于绝对加速度谱，伪速度谱能更清楚地显示出结构在低频、中频和高频段不同的冲击响应特征。分析了弹性力和惯性力在低频、中频和高频段对结构安全性的影响，据此在对数四坐标伪速度谱上给出了相应的结构破坏边界。以一典型蜂窝夹层结构为研究对象，通过有限元分析计算得到的结构破坏边界与伪速度谱给出的结构破坏边界符合得较好。在航天器结构冲击安全性研究领域，本文采用的伪速度谱结构冲击破坏边界是对目前常用的加速度谱方法的一个有益补充。     

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。