槽道射流及端壁抽吸对角区分离的组合控制研究

为优化叶片吸力面流动分离结构,探究对于角区分离更好的流动控制方法,以一大弯角扩压静子叶栅为研究对象,对叶片进行全叶高槽道结构处理,并在其基础上于槽道出口前进行端壁抽吸槽结构处理.在来流马赫数为0.7,来流攻角为-8°～6°工况下,对原型叶栅、全叶高开槽叶栅及组合流动控制叶栅进行性能计算及对比.结果表明:全叶高开槽方案能...     

低雷诺数仿生分离流翼型气动特性初探

为了探索适合低雷诺数微型飞行器的翼型形式,基于对自然界鸟类和昆虫滑翔飞行时翅膀形状的观察,设计出一种由前缘削尖平板和后缘圆弧翼型组合而成的仿生分离流翼型。数值研究结果表明,气流在削尖平板的前缘点强制分离,形成大范围低压分离流动,随后在后部圆弧翼上表面再附形成稳定低压涡流区,从而实现较高的气动效率和较强的抵抗大气湍流的能力。上削尖平板可以使流动分离点固定在削尖点。相对于单独平板,仿生分离流翼型的升力系数有大幅提高,迎角为4°时提高了112%。此外,仿生分离流翼型可以在较宽的迎角范围内（4°~20°）保持高升力,但是迎角增加,阻力也快速增大,因此小迎角情况下（小于4°）气动效率更优。      

两点法测量直线度中传感器对齐误差的探讨

针对以往关于两点法测量直线度的文献中要求两传感器端部严格对齐的问题,进行了数学分析和计算机仿真,证明对齐误差并不影响最后的误差分离准确度,同时可在一定程度上降低对传感器安装误差的要求。     

仿生翅室对跨声速扩压叶栅角区分离流动影响研究

为了抑制压气机叶片吸力面角区分离,减小内部流动损失,改善通道内的通流能力,基于蜻蜓翅翼的翅室和褶皱结构特征,在跨声速扩压叶栅的端壁上布置仿生翅室结构.采用数值模拟方法,研究不同深度的仿生翅室结构对角区分离流动的影响.研究结果表明:0°攻角条件下仿生翅室影响效果最明显,能够提高端壁附近的湍动能,增加靠近端壁处流体速度,减...     

Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.     

基于KBE的飞机板金件工艺性审查系统

由于板金零件的可成形性取决于多方面的因素,板金零件成形的工艺性审查也就显得十分复杂,工艺审查的合理性和准确性往往成为飞机设计和制造的矛盾焦点.通过分析当前我国飞机板金零件工艺性审查的现状,提出了在工艺性审查中利用基于知识的(KBE,Knowledge Based Engineering)技术的必要性.分析了利用后台数据库及知识库创建工艺性审查系统的总体结构和实现方案,并对系统创建中的关键技术及解决方法进行了研究.通过实例验证了该系统的功能及可靠性.      

An empirical model of the plasma environment around Mercury

Since the flyby observations by Mariner 10 in 1974 and 1975, Mercury has been one of the most interesting objects for space physics and planetary exploration. The MESSENGER and BepiColombo missions now plan to revisit this planet. In order to design plasma instruments for the BepiColombo mission, we have estimated electron and ion fluxes around Mercury with an empirical model, which has been developed for the Earth’s magnetotail. The solar wind data needed as input parameters are derived from Helios observations. The result shows that our predicted electron fluxes at aphelion agree well with the Mariner-10 data. It is also noted that ion instruments must cover a very wide dynamic range of proton fluxes. However, the applicability of the Earth’s magnetospheric model to Mercury is, in itself, an important issue for comparative magnetospheric studies.     

基于盲源分离技术的航空发动机振动信号分析

基于双转子航空发动机机匣拾取振动信号特征的分析,采用基于数学形态学滤波前处理的盲源分离识别方法进行特征提取.针对机匣拾取振动信号的特征,利用开—闭和闭—开组合数学形态滤波器在保留信号基本形状的前提下,滤除掉原始信号中的噪声分量.利用Fast ICA算法恢复高、低压转子源振动信号的波形.对实测数据的分析表明,该方法能够较好地恢复高、低压转子所激振动信号的频域结构信息,有利于提高故障定位的准确性.     

Understanding Substorms in the Magnetotail: Early Development and Recent Progress

This is a concise review of physics of the substorm in the magnetotail. It consists of two parts. The first part summarizes historical developments in the early days of the space age (1960--1975) when the basic concepts such as magnetotail and reconnection were established and the leading model of the substorm was introduced. The second part is an overview of the research conducted in recent years (1995--2010) when very significant advances have been achieved in understanding the substorm physics by virtue of several major satellites missions that addressed the magnetotail physics intensively.      

前缘吹气控制舵面流动分离

针对各种飞行器大舵偏下出现的流动分离问题,在北航D4风洞对旨在消除舵面流动分离的舵面前缘吹气技术进行了研究,为了降低控制分离所用的吹气量,吹气点设置在舵面前缘气流分离点处.应用粒子图像测速(PIV,Particle Image Velocimetry)技术,分析了舵面绕流在吹气量由小变大过程中所经历的3个不同演化阶段;由测压得到的舵面压力分布则显示,前缘吹气造成的引射作用使前缘吸力峰随吹气量增大而增大,这是前缘吹气能够使舵面升力增大的主要机理.实验结果还表明,前缘吹气可明显提高舵面升力,同时也可以显著降低舵面阻力.