襟翼不对称运动和襟翼倾斜的保护逻辑研究

实现高升力系统的故障保护对提高电传飞机安全性具有重要的意义.本文描述了高升力系统后缘襟翼的架构;针对不对称故障和倾斜故障的监控和和保护方式问题,分析了上述两类故障的监控和保护措施及其工作逻辑,在确定工作逻辑的阈值参数时综合考虑了检测和确认故障、襟翼动力驱动装置的制动过程以及系统机械误等因素;建立了故障保护逻辑的Simulink模型,并对不同的失效情况进行了仿真分析,仿真结果表明本文设计的故障保护措施能够很好地监控系统并防止故障蔓延,研究结果对民机高升力系统设计具有一定的借鉴意义.     

加速度计全量程标度因数不对称性标定算法研究

全量程标度因数不对称性是高精度石英挠性加速度计的一项重要指标,其大小对于惯导系统的导航精度具有非常大的影响。在加速度计精密离心机测试中,由离心加载引起的各种误差是进行加速度计标定的主要影响因素,论文给出了适用于精密离心机测试的加速度计输出模型与数据求解方法。为提高标定精度,以标度因数测试误差作为衡量指标,对输入数据进行迭代与修正;对修正后的测试数据进行三阶拟合,计算正向与负向标度因数,从而得到全量程标度因数不对称性。经试验验证,测试数据修正后可将标度因数误差从10-4降低至10-9,标度因数不对称性水平从10-4提高至10-5。     

基于性能退化缓解的双发推力匹配控制

为了解决退化程度不同而导致的双发推力不匹配问题,首先介绍基于发动机性能退化缓解控制的双发推力匹配控制系统(在发动机基准控制系统的基础上添加外围控制回路实现对推力的间接控制,并通过设定双发共同遵循的期望推力减少由于发动机退化程度不同造成的双发推力差异),之后对该系统所涉及的推力设定、参数估计、转速指令修正等关键技术进行研究,最后在MATLAB/Simulink环境下进行仿真验证,结果表明:该系统可以在发动机参数限制范围内合理地设定双发共同遵循的期望推力,减少推力差异,满足自动协调双发推力匹配的设计要求。     

可压缩流中声激励对细长体大迎角流动非对称性的影响研究

在跨声速风洞中研究了声激励对于可压缩流中细长旋成体大迎角流动非对称性的影响效果。结果表明,在可压缩流场中,声激励对于细长体典型迎角下的流动非对称性依然有着一定的影响,但由于高速风洞中流场本身的湍流度较高,声激励效果要比低湍流度不可压缩流中的影响弱。     

Investigation of N–S asymmetry of solar differential rotation by various patterns for solar cycles 20 and 21

For solar cycles 20 and 21 the latitudinal variations of the solar rotation rates are found using data of the H_α filaments and the long-lived magnetic features of negative and positive polarities. Analysis of the data showed that: (a) there is N–S asymmetry in the equatorial rotation of the H_α filaments and the long-lived magnetic features; (b) for both solar cycles the long-lived magnetic features of both polarities have similar behavior; (c) in the solar cycle 20 the long-lived magnetic features of both polarities vary in phase to each other but show some difference during cycle 21. For the long-lived magnetic features of positive polarity the confidence level is lower than for those of negative one.     

The asymmetrical features in electron density during extreme solar minimum

The variations of plasma density in topside ionosphere during 23rd/24th solar cycle minimum attract more attentions in recently years. In this analysis, we use the data of electron density (Ne) from DEMETER (Detection of Electromagnetic Emissions Transmitted from Earthquake Regions) satellite at the altitude of 660–710 km to investigate the solstitial and equinoctial asymmetry under geomagnetic coordinate system at LT (local time) 1030 and 2230 during 2005–2010, especially in solar minimum years of 2008–2009. The results reveal that ΔNe (December–June) is always positive over Southern Hemisphere and negative over northern part whatever at LT 1030 or 2230, only at 0–10°N the winter anomaly occurs with ΔNe (December–June) > 0, and its amplitude becomes smaller with the declining of solar flux from 2005 to 2009. The ΔNe between September and March is completely negative during 2005–2008, but in 2009, it turns to be positive at latitudes of 20°S–40°N at LT 1030 and 10°S–20°N at LT 2230. Furthermore, the solstitial and equinoctial asymmetry index (AI) are calculated and studied respectively, which all depends on local time, latitude and longitude. The notable differences occur at higher latitudes in solar minimum year of 2009 with those in 2005–2008. The equinoctial AI at LT 2230 is quite consistent with the variational trend of solar flux with the lowest absolute AI occurring in 2009, the extreme solar minimum, but the solstitial AI exhibits abnormal enhancement during 2008 and 2009 with bigger AI than those in 2005–2007. Compared with the neutral compositions at 500 km altitude, it illustrates that [O/N₂] and [O] play some roles in daytime and nighttime asymmetry of Ne at topside ionosphere.     

On radiation belt dynamics during magnetic storms

Temporal variations of the radiation belt particle during the magnetic storms are investigated using measurements by the low altitude satellite spectrometer. Along with several known effects, such as the outer radiation belt intensity decrease at the main phase, the radial diffusion with the particle acceleration and the recovery of the radiation belt during the recovery phase, some less known features were investigated, such as the dawn–dusk asymmetry of the radiation belt.     

方管内超声速湍流流动及旋涡的测定技术研究

本文在Ｍ∞＝１．５８及湍流边界层厚度δ／Ｄ＝０．１条件下，用实验方法研究了管长Ｌ／Ｄ＝６方管内的三维超声波湍流场及其沿程的发展和反压的影响，讨论了壁面边界层沿流向和展向的主要变化特征；指出管内横截面的三维静压场特点，文中最后探讨了超声速湍流流动的方管内旋涡的测量技术。     

细长旋成体大迎角非对称流动特性的试验研究

简要介绍了细长体大迎角流动非对称性的试验结果,分析了Re数、湍流度和安装条件等因素对大迎角流动非对称性的影响,探讨了大迎角流动非对称性的产生机制。文章最后着重阐述了该研究得出的一些支持细长体大迎角流动非对称性产生机制的空间动力不稳定性观点的理由。     

背风涡隔离对大攻角旋成体表面压力分布的影响

通过在背风母线处沿纵向对称面嵌入隔离板，观测了大攻角旋成体在这种背风涡被隔离状态下的表面压力分布情况。隔离板的作用旨在削弱、隔阻两侧背风涡间的相互联系和诱导，以便考察背风涡诱导作用对物面流动的影响。不同隔离（包括无隔离情况）状态下的实验结果表明，背风涡的隔离对表面压力分布有不同程度的影响，故这一研究和结果可供探讨大攻角流动非对称性成因作参考。