开槽尾流板对跨声速涡轮平面叶栅流场影响的实验

采用数值计算和实验相结合的方式研究了开槽尾流板对跨声速涡轮平面叶栅流场周期性的影响。通过数值计算研究了不同开孔率（10%、15%、30%、50%）和偏转角度（70°、71°、72°）下尾流板对叶片表面及叶栅流道出口压力分布的影响,并通过实验验证了尾流板对流道出口流场周期性的改善作用。结果表明:无尾流板时叶片表面压力分布明显偏离周期性计算结果,且流道出口压力分布的周期性误差较大;尾流板偏转角度和开孔率会影响叶片表面及叶栅流道出口的压力分布,适当调节尾流板参数能改善流场周期性;安装开孔率为50%,偏转角度为70°的尾流板时各流道出口的压力分布一致性最好且最接近周期性计算结果,计算和实验结果的周期性误差较无尾流板时分别降低47.6%和28.1%。      

考虑磁滞效应的电抗器二维电磁场计算

将JA模型与电磁场数值分析方法相结合,在考虑铁心的磁滞效应的情况下,推导出电磁场的有限元计算模型。分别采用基本磁化曲线和磁滞回线两种不同的方法对电抗器的电磁场进行仿真计算。研究结果表明磁滞现象对电抗器电磁场的计算影响较大,因此考虑磁滞效应的电磁场数值计算模型,为进一步研究电抗器的发热问题奠定了理论基础。     

惯导平台长时间通电有限元热分析

长时间通电会造成惯导平台腔内温度场发生较大变化,鉴于惯性仪表对环境场的敏感性,温度的变化将极大影响平台的性能。通过某型气浮惯导平台长时间通电温度场变化有限元热分析,建立了通电时间与平台各部件温度场模型、平台腔内温度场模型以及台体耦合的热弹性结构模型,得到了温度场分布的量化结果,分析了平台台体的热应力分布情况。在温度数据的处理过程中,利用Matlab构建数据模型,预测了各部件及腔内的温度变化趋势,并通过对比试验数据,验证了仿真结果的正确性,为后续研究提供了理论基础。     

机场条件对民机起飞性能影响规律初探

为了研究机场海拔、温度及跑道污染对大型民航运输机起飞性能的影响规律,采用理论分析结合模型计算的方法,回归统计出机场条件对起飞场长的影响规律。首先,介绍并分析了起飞性能的影响要素(机场高度、温度、跑道条件、发动机推力、增升装置)及其影响关系;其次,建立了自动满足适航要求的民机起飞性能计算模型;再次,利用该模型计算不同机场条件下飞机起飞性能;最后,将结果分析归纳总结成图表,为飞机设计及运营人员提供参考。     

民用飞机试验件制造检查项目的推荐及确定

在民用飞机适航取证过程中,申请人需通过制造符合性检查以保证生产制造各类型试验件及其生产过程符合经批准的型号设计资料。审查方通过申请人推荐制造符合性检查项目确定需要经过检查的试验件。从民用飞机制造符合性检查的流程着手,定义制造符合性检查项目、项目推荐原则以及推荐过程中项目的检查属性等,并从生产质量控制、构型控制两方面分析制造符合性检查项目推荐过程中需要关注的重点。     

U型无铁心永磁同步直线电机磁场建模与分析

传统的铁心式直线电机由于铁心开断的影响,造成了横向和纵向边端效应,使推力输出波动较大;无铁心永磁直线电机具有零齿槽效应的优点,结构简单,控制灵活。采用两种解析法求解无铁心永磁同步直线电机气隙磁场的问题,即等效磁势法和等效磁化电流法,同时采用有限元法对电机磁场进行有限元分析,验证解析法磁场解析计算的准确性。最后分析电机主要尺寸对气隙磁场的影响。通过改变电机参数,进行了优化设计,为同类电机的设计与分析提供了参考。     

Simulation-based evaluation of a cold atom interferometry gradiometer concept for gravity field recovery

The prospects of future satellite gravimetry missions to sustain a continuous and improved observation of the gravitational field have stimulated studies of new concepts of space inertial sensors with potentially improved precision and stability. This is in particular the case for cold-atom interferometry (CAI) gradiometry which is the object of this paper. The performance of a specific CAI gradiometer design is studied here in terms of quality of the recovered gravity field through a closed-loop numerical simulation of the measurement and processing workflow. First we show that mapping the time-variable field on a monthly basis would require a noise level below $5\text{mE}/\sqrt{\text{Hz}}$. The mission scenarios are therefore focused on the static field, like GOCE. Second, the stringent requirement on the angular velocity of a one-arm gradiometer, which must not exceed ${10}^{-6}$?rad/s, leads to two possible modes of operation of the CAI gradiometer: the nadir and the quasi-inertial mode. In the nadir mode, which corresponds to the usual Earth-pointing satellite attitude, only the gradient $V_{\mathit{yy}}$, along the cross-track direction, is measured. In the quasi-inertial mode, the satellite attitude is approximately constant in the inertial reference frame and the 3 diagonal gradients $V_{\mathit{xx}}\text{,}{V}_{\mathit{yy}}$ and $V_{\mathit{zz}}$ are measured. Both modes are successively simulated for a 239?km altitude orbit and the error on the recovered gravity models eventually compared to GOCE solutions. We conclude that for the specific CAI gradiometer design assumed in this paper, only the quasi-inertial mode scenario would be able to significantly outperform GOCE results at the cost of technically challenging requirements on the orbit and attitude control.     

A study of a long duration B9 flare-CME event and associated shock

We present and discuss here the observations of a small long duration GOES B-class flare associated with a quiescent filament eruption, a global EUV wave and a CME on 2011 May 11. The event was well observed by the Solar Dynamics Observatory (SDO), GONG H$\alpha$, STEREO and Culgoora spectrograph. As the filament erupted, ahead of the filament we observed the propagation of EIT wave fronts, as well as two flare ribbons on both sides of the polarity inversion line (PIL) on the solar surface. The observations show the co-existence of two types of EUV waves, i.e., a fast and a slow one. A type II radio burst with up to the third harmonic component was also associated with this event. The evolution of photospheric magnetic field showed flux emergence and cancellation at the filament site before its eruption.     

磁拓扑结构对环型离子推力器放电性能的影响

为得到环型离子推力器最佳磁拓扑结构以有效提高推力器放电效率、降低放电损耗,对不同类型磁拓扑结构下的放电通道气体放电过程进行研究。采用PIC MCC数值计算方法对等离子体产生及运输过程进行数值模拟,分析磁场分布对等离子体密度分布、电子损耗率及放电稳定性的影响,结合统计结果,得到推力器放电性能曲线,最后进行试验验证。研究结果表明,相较多极场结构,环尖场磁构型能更好地约束电子运动,大幅降低其在阳极壁面损耗率,增加电子与中性原子碰撞概率,显著提高放电效率、降低放电损耗。     

磁悬浮控制敏感陀螺转子前馈解耦内模控制

磁悬浮控制敏感陀螺以洛伦兹力磁轴承（LFMB）为力矩器驱动转子偏转。针对磁悬浮控制敏感陀螺转子径向转动自由度间存在耦合的问题以及转子偏转高精度快响应要求,提出一种前馈解耦内模控制方法。根据洛伦兹力磁轴承的工作原理建立了转子偏转动力学模型,并设计了前馈解耦矩阵实现转子径向偏转解耦,在此基础上,采用二自由度内模控制器（2-DOF IMC）对转子进行高精度快响应偏转控制。MATLAB仿真结果表明所提出的控制方法可有效实现对陀螺转子偏转的完全解耦,且转子偏转响应时间较交叉PID算法减少57.1%,受0.1sin（2πt）°正弦信号扰动影响产生的偏转波动幅值较交叉PID算法减少76%。