风对建筑绕流流动的数值方法

本文利用k-ε湍流模型及SIMPLE方法,在二维条件下,就风对建筑绕流流动进行了数值模拟,建筑及地面的边界条件采用以低Re数k-ε湍流模型中导出的壁函数处理近壁湍流。自由边界采用外推格式。对于计算域中的建筑物则利用控制粘性系数的方法处理。并对计算结果和风洞实验进行了比较。 为了研究建筑物之间的气流及压力分布,本文还对并列两栋建筑的不同情况进行了数值计算和分析。     

矩形风洞收缩段流场的计算和分析

本文结合西工大低速风洞设计进行了矩形三元收缩段流场的计算和分析,计算采用差分方法和贴体坐标,以AF1格式进行离散化并利用ADI方法求解。对三种常用的收缩曲线(即Witozinsky曲线,五次方曲线和双三次方曲线)的三元流场进行了具体计算和比较。计算结果正确反映了三元收缩段流动的特点,给出了流动三元性对壁面逆压梯度和出口均匀性影响的数值结果,表明本文方法是三元收缩段设计的有效分析和设计手段。     

EXPERIMENTAL RESEARCH OF THE CONFIGURATION OF WING－TIP DRAG REDUCTION FOR LIGHT AIRCRAFT

ＥＸＰＥＲＩＭＥＮＴＡＬＲＥＳＥＡＲＣＨＯＦＴＨＥＣＯＮＦＩＧＵＲＡＴＩＯＮＯＦＷＩＮＧ－ＴＩＰＤＲＡＧＲＥＤＵＣＴＩＯＮＦＯＲＬＩＧＨＴＡＩＲＣＲＡＦＴＤｅｎｇＹａｎｍｉｎ，ＨｕＪｉｚｈｏｎｇ（ＦａｃｕｌｔｙｏｆＬｉｇｈｔＡｉｒｃｒａｆｔＤｅｓｉｇ...     

Broadening of Fe X (6374 Å) profiles above the limb in a coronal hole

Profiles of the visible Fe X (6374 Å) coronal emission line as a function of height above the limb were obtained out to 1.16 solar radii in a coronal hole using the NSO/Sacramento Peak Observatory Coronagraph, Universal Spectrograph and a CCD camera. These are the first coronal line profiles obtained as a function of height in a coronal hole from the ground. Analysis of the line widths suggests a large component of nonthermal broadening which increases with height ranging from 40 to 60 km/s, depending upon the assumed temperature or thermal component of the profile.     

低RCS飞行器外形设计实践

 在鸭式布局的基础上 ,对飞行器各部件及部件间的连接方式进行了外形隐身设计。对初步形成的鸭翼 -翼身融合体改变机身头部形状和立尾配置等进行 RCS优化。给出了飞行器各种状态下的 RCS平均值和迎头± 45°区内的 RCS值。测试结果表明 ,尖头机身、 30°双立尾 (立尾与垂直平面成± 30°角 )的鸭翼 -翼身融合体的 RCS值最小。对 RCS优化后的外形 ,风洞测力试验表明其气动性能也较好 (最大升阻比达到 8,失速迎角超过 2 6°)     

SDM 标模大攻角动导数试验

介绍了ＣＡＲＤＣ高速所１．２ｍ风洞大攻角的动导数试验装置与测量系统以及在１．２ｍ风洞中对标准动态模型（ＳＤＭ标模）所作的一系列风洞试验结果。试验结果与国外文献数据具有较好的一致性。试验结果随马赫数和攻角的变化表现出明显的非线性,而减缩频率的影响并不显著。天平与测试系统的重复性精度较高。     

Global Response of Martian Plasma Environment to an Interplanetary Structure: From Ena and Plasma Observations at Mars

As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485 of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic flux variations of the ENA flux at the spacecraft location.     

98RK电子压力扫描系统在NH-1风洞中的应用

美国PSI公司开发的98RK电子压力扫描系统作为一种高速高精度多用途的自动测量仪器,在风洞试验中具有很高的使用价值。本文介绍了该系统的结构性能和在NH—l风洞中的应用。     

三维舵面绕流的N-S方程计算研究

基于粘性非结构混合网格,采用格心格式的有限体积法,应用Spalart-Allmaras湍流模型进行绕三维舵面流动的N-S方程数值模拟。操纵面铰链力矩的计算结果与风洞试验结果的对比分析表明,计算方法对粘性流动具有良好的适应性。对舵面铰链力矩随迎角、马赫数、雷诺数变化的规律也进行了分析研究。