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.     

非对称来流下隔离段动态压力特性

为了探讨非对称来流下矩形隔离段内动态压力特性,用直联实验方式以及动态压力测量技术进行了试验,并用统计分析方法分析了数据。实验结果表明,入口来流的非对称性对上下壁面压力脉动大小以及传播平均速度有较大影响,而对频率无多大影响。激波串区域内壁面压力脉动向下游传播比向上游传播衰减得快。在隔离段出口超声速条件下,观测到的压力脉动频率主要在70 Hz以下,而在出口亚声速条件时,压力脉动的频率不仅有70Hz以下的部分,而且还有100~200 Hz之间的部分。     

超声速进气道喉部附面层抽吸

为研究超声速进气道喉部之后流场激波附面层干扰,采用FLUENT软件模拟了单楔角进气道在设计工况下流动情况。通过分析,提出进气道喉部抽吸。计算了三种抽吸缝大小下进气道喉部之后流场,计算结果表明,喉部抽吸能使激波稳定于喉部,通过抽吸能改善喉部之后流场状况,提高进气道性能,少量抽气不改变流场结构,加大抽气量,使喉部之后激波串转变成正激波,正激波之后流场不分离,进气道出口性能参数提高显著。     

几种超声速非常规压缩系统的研究

根据斜激波和膨胀波理论,数值计算得到给定非常规压缩型面所形成的弯曲激波型面和壁面静压分布,同Fluent计算结果进行比较。应用Fluent软件,计算了等压力梯度设计非常规曲面压缩二元进气道、常规等熵压缩二元进气道和三楔压缩二元进气道设计点性能。研究结果表明:数值计算得到的弯曲激波型面与Fluent计算结果吻合较好。等压力梯度设计的非常规压缩型面壁面静压均匀上升,有利于防止壁面附面层分离;其压缩面长度比等熵压缩面缩短21.6%,减轻了进气道的重量。     

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.     

SFD方法模拟高超声速进气道中激波与边界层干扰

采用ＳＦＤ方法,在ＥＸＣＥＬ软件上利用ＮＮＤ格式数值模拟了激波与平板边界层之间的相互作用以及激波与管道壁面边界层的相互作用,即高超声速进气道隔离段内激波串流动现象。该方法的特点是简单、直观而且不用常规编程,计算结果基本反映了流场的基本结构,表明ＳＦＤ方法是一种具有潜力的计算方法。     

冲击温度的理论计算及分析

当空间飞行器受到碎片的碰撞时,其壳体中会产生冲击加热。文章概述了计算冲击温度的三种基本方法;计算了铁的冲击加热温度,并与实验测量值作了比较。结果表明,利用三项式物态方程计算的冲击温度与测量值符合得比较好。另外,还对影响冲击温度计算值的若干因素进行了分析     

具有无源控制空腔时正激波/湍流附面层干扰的数值模拟

采用雷诺平均N-S方程和B/L代数湍流模型计算了具有无源控制空腔时正激波/湍流附面层干扰流场。计算与实验结果的比较表明,本文方法可较准确地预测激波结构、激波与附面层干扰区流动基本特征及波后流动分离状态、激波位置、波前马赫数等参数。      

关于建立高阶差分格式的问题

为了能在不太密的网格上捕捉到流场的细致结构。通常采用高阶精度的差分 式进行数值模拟。为能抑制计算中和在激波附近产生的虚假波动,本文从物理构思出发,提出了建立高阶格式的两个基本原则,作者称之为抑制波动的原则和稳定性原则。