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。     

燃气轮机系统仿真集成概念及其分布对象实现

本文提出燃气轮机系统仿真集成的概念, 分析了关键实现技术, 然后从跨平台性入手, 给出 1个分布异构计算机平台上的面向对象实现方案。算例表明, 这一方案成功实现了系统仿真集成的主要功能, 从而为发动机系统的多学科开发、研制和实验提供了有效的仿真软、硬件平台, 并使发动机的远程协同设计成为可能。      

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.     

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。     

平流层长航时气球轨迹控制系统研究

首先介绍了平流层气球的应用意义及进行轨迹控制的必要性,然后描述了一种基于不同海拔风速差的轨迹控制方法,简要说明了平流层风速随海拔的变化规律,在此基础上研究了包括超压气球和轨迹控制系统在内的气球飞行系统各部分特点,最后简单分析了整个飞行系统的建模与仿真中的要点问题。结果表明,这种轨迹控制方法是一种几乎不需要消耗能源的有效轨迹控制方法,具有较高的应用价值和推广价值。