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。     

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。     

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。     

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.     

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。     

Solar cycle variation of “killer” electrons at geosynchronous orbit and electron flux correlation with the solar wind parameters and ULF waves intensity

To construct models for hazard prediction from radiation belt particles to satellite electronics, one should know temporal behavior of the particle fluxes. We analyzed 11-year variation in relativistic electron flux (E>2 MeV) at geosynchronous orbit using measurements made by GOES satellites during the 23rd sunspot cycle. As it is believed that electron flux enhancements are connected with the high-speed solar wind streams and ULF or/and VLF activity in the magnetosphere, we studied also solar cycle changes in rank order cross-correlation of the outer radiation belt electron flux with the solar wind speed and both interplanetary and on-ground wave intensity. Data from magnetometers and plasma sensors onboard the spacecraft ACE and WIND, as well as magnetic measurements at two mid-latitude diametrically opposite INTERMAGNET observatories were used. Results obtained show that average value of relativistic electron flux at the decay and minimum phases of solar activity is one order higher than the flux during maximum sunspot activity. Of all solar wind parameters, only solar wind speed variation has significant correlation with changes in relativistic electron flux, taking the lead over the latter by 2 days. Variations in ULF amplitude advance changes in electron flux by 3 days. Results of the above study may be of interest for model makers developing forecast algorithms.     

Composition Variations in the Solar Corona and Solar Wind

Order of magnitude variations in relative elemental abundances are observed in the solar corona and solar wind. The instruments aboard SOHO make it possible to explore these variations in detail to determine whether they arise near the solar surface or higher in the corona. A substantial enhancement of low First Ionization Potential (FIP) elements relative to high FIP elements is often seen in both the corona and the solar wind, and that must arise in the chromosphere. Several theoretical models have been put forward to account for the FIP effect, but as yet even the basic physical mechanism responsible remains an open question. Evidence for gravitational settling is also found at larger heights in quiescent streamers. The question is why the heavier elements don't settle out completely. This revised version was published online in June 2006 with corrections to the Cover Date.     

建筑物行人高度风环境风洞试验研究

介绍了建筑物风环境的风洞模拟，行人高度风测量探头的设计、标定和数据处理。采用这种探头，在气动中心低速所４ｍ×３ｍ风洞的长１５ｍ、宽４ｍ、高２．２ｍ风工程试验段进行了比例为１∶３００的建筑群模型的行人高度风环境试验研究，结果说明这座新高层建筑物的落成，对其周围某些位置的行人高度风环境有严重的影响。     

多加速度计振动分离惯性补偿测力技术

为解决在高超声速脉冲风洞中进行大长细比等特殊模型测力实验所面临的惯性补偿问题,笔者提出了多加速度计振动分离惯性补偿方法。这一方法应用在长细比达20 :1 的模型气动力实验中,得到了较为理想的实验结果     

基于VXI总线的高速风洞脉动压力测试与分析系统

VXI总线代表着当今自动测试领域的发展方向。笔者介绍了气动中心高速所组建的基于VXI总线的高速风洞脉动压力测试系统,文中给出了测试仪器的计量指标,并简要说明了测量与分析软件的开发过程。通过风洞试验的实际检验,表明该套系统性能先进,稳定可靠,具有广泛的应用前景