基于激光多普勒原理的极低风速测量实验

介绍了利用激光多普勒效应进行风速测量的原理及定点遥测原理,分析了探测气溶胶颗粒大小的要求,并以此搭建了一套极低风速测量系统。同时分析了系统的测速精度,以及安装角度对测量结果的影响。最后分别开展了转台实验、直线导轨实验和风洞实验,实验结果表明,该极低风速测量系统的测量误差基本可以控制在001 m/s以内,当风洞工作介质为未经处理的环境空气时,系统可以获得稳定可靠的信号,测量结果与高性能仪器十分接近。     

0.3 m低温风洞液氮供给系统研制

基于系统级的一维热流体模拟分析,建立了适用于研究分析0.3 m低温风洞液氮供给系统的数学模型,并开展了系统漏热、两相流及缓冲罐中液氮容积等流体动力学分析;在系统现有控制策略及试验数据的基础上,基于该数学模型开展了系统压力动态响应分析,获得了在阀门动态调节过程中管网压力的瞬态响应,计算结果与试验值的总体误差控制在10%以内。喷射压力一致化改造避免了阀间干扰,添加的回流管道消除了供给末端的两相流现象,使喷射压力控制精度达到1.1%,调节时间减少到23 s,实现了风洞总温快速安全调节和精确控制。     

Advances in critical technologies for hypersonic and high-enthalpy wind tunnel

Hypersonic and high-enthalpy wind tunnels and their measurement techniques are the cornerstone of the hypersonic flight era that is a dream for human beings to fly faster, higher and further. The great progress has been achieved during the recent years and their critical technologies are still in an urgent need for further development. There are at least four kinds of hypersonic and high-enthalpy wind tunnels that are widely applied over the world and can be classified according to their operation modes. These wind tunnels are named as air-directly-heated hypersonic wind tunnel, light-gas-heated shock tunnel, free-piston-driven shock tunnel and detonation-driven shock tunnel, respectively. The critical technologies for developing the wind tunnels are introduced in this paper, and their merits and weakness are discussed based on wind tunnel performance evaluation. Measurement techniques especially developed for high-enthalpy flows are a part of the hypersonic wind tunnel technology because the flow is a chemically reacting gas motion and its diagnosis needs specially designed instruments. Three kinds of the measurement techniques considered to be of primary importance are introduced here, including the heat flux sensor, the aerodynamic balance, and optical diagnosis techniques. The techniques are developed usually for conventional wind tunnels, but further improved for hypersonic and high-enthalpy tunnels. The hypersonic ground test facilities have provided us with most of valuable experimental data on high-enthalpy flows and will play a more important role in hypersonic research area in the future. Therefore, several prospects for developing hypersonic and high-enthalpy wind tunnels are presented from our point of view.     

基于正交优化设计的诱导轮空化性能研究

为了研究不同结构因素对诱导轮空化性能的影响及主次顺序,基于正交优化设计,采用数值模拟的方法,通过诱导轮可视化试验进行验证,对某型诱导轮及其改型进行了分析。仿真计算得到的不同空化数下空穴形态与实验结果吻合较好,断裂空化数的计算结果与实验结果误差为0.3%。仿真及实验结果表明,诱导轮发生扬程断裂不仅与空穴区占流道体积的大小有关,还与空穴区在流道中分布的位置有关,空穴区位置越靠后,越容易发生扬程断裂;对诱导轮空化性能及水力效率影响最大的结构因素为入口安放角,其次为入口修圆包角;入口等螺距段长度和变螺距段长度较小时可以提高诱导轮的空化性能。     

舰载直升机理论风限图飞行模拟获取方法

获取舰载直升机实用风限图,仅依靠实装飞行试验或建模仿真都是非常困难的。通过起降飞行模拟试验获取理论风限图,结合少量的海上实装飞行验证试验是一种综合较优的方法。起降飞行模拟试验需要真实飞行员和高等级飞行模拟器参与,飞行模拟器中的母舰气流场数据、母舰运动可由建模仿真或试验测试得到,且必须考虑母舰气流场的非定场特性;只有当飞行员视景或视觉反馈受限时(如能见度降低时),飞行模拟器基座的六自由度运动才是必需的;用DIPES或Bedford方法量化飞行员主观操纵负担,结合记录的客观操纵数据,评判起降难度;典型的飞行模拟试验程序包含了不同风况下的进近和甲板着舰,通常每隔15°和5kn一个风况。通过起降飞行模拟试验得到的理论风限图,可以更加有效和安全地指导海上实装飞行验证试验,最终获得实用风限图。     

共轴式直升机桨毂阻力特性与减阻试验

共轴式直升机桨毂阻力占全机废阻的50%以上,因此有必要对桨毂阻力特性和减阻设计进行研究。 通过对某共轴式直升机桨毂模型、减阻方案及减阻方案加装涡流发生器进行风洞试验,研究轴式直升机桨毂的 阻力特性,验证减阻方案及减阻方案加装涡流发生器的减阻效果。结果表明:桨毂支臂方位角、转速和攻角变 化对桨毂及其减阻方案的阻力影响很小;上下桨毂整流罩与中间轴整流罩之间的缝隙对阻力影响比较大;减阻 方案可以降低约33%的桨毂阻力,而加装涡流发生器的减阻效果并不明显。     

大型双曲冷却塔表面脉动风压随机特性——风压极值探讨

针对风压信号呈现的非高斯特性和传统极限估计方法的局限,首次提出基于保证率和相关性的极值估计方法——全概率迭代法进行冷却塔表面脉动风荷载极值分析,并和传统的峰值因子法及改进的Sadek-Simiu法计算结果进行对比验证。结果表明：全概率迭代法避开了对随机过程的高斯分布假定,相比传统的极值估计方法其结果更加真实可靠;表达风压极值中脉动分量的峰值因子数值沿着环向和子午向变化显著,如取为同一数值则偏于危险或过于保守;采用全概率迭代法得到的表面风压系数极值分布曲线与规范取值相比,迎风面和负压峰值区域极值偏小,背风区域极值偏大,且最小值对应角度相差约10°。     

Geomagnetic activity driven by solar wind turbulence

Within the framework of the solar wind—magnetosphere coupled system, intense perturbations in the solar wind, causing geomagnetic storms and substorms, have been widely studied by means of the so-called coupling parameters. However, remarkable variations in the geomagnetic field occur even in absence of such perturbations. In those conditions, solar wind MHD turbulence might have a role. Recent results have shown that solar wind turbulence can be described not only as a mixture of inward and outward stochastic Alfvénic fluctuations, but includes also advected structures, dominated by an excess of magnetic energy.     

The effects of the solar magnetic polarity and the solar wind velocity on Bz-component of the interplanetary magnetic field

We have studied the effect of both solar magnetic polarity and the solar wind velocity on the Bz-component of the interplanetary magnetic field, IMFBz, for the minimum activity of the solar cycles 21, 22, 23 and 24. We made a statistical study of IMFBz in the first section which is considered as an extension of Lyatsky et al. (2003). They made a statistical study of IMFBz for two periods of minimum solar activity 22 and 23 related to 1985–1987 and 1995–1997 when the solar magnetic field had opposite polarity. Our results seem to be consistent with the results obtained by Lyatsky et al. (2003). We found that there is a dependence of IMFBz on the IMFBx and the solar magnetic polarity for the minimum periods of the selected four solar cycles. In addition, we found that there is a dependence of IMFBz on the solar wind velocity.     

风力机组叶片的先进翼型族设计

大型风力机组叶片设计需要专用的翼型族,以满足风力机组运行的环境要求。高升阻比、低粗糙度影响是该翼型族的气动性能特点。为了发展我国具有自主知识产权的风力机专用翼型族,在科技部863项目的支持下,北京航空航天大学联合国内气动研究单位,通过理论分析、数值模拟和风洞试验等技术途径,开发了两个适用于大型风力机组叶片的先进翼型族。理论分析和风洞试验表明,设计结果基本达到了预先设定的气动性能指标。