航空结构件铣削残余应力分布规律的研究

 采用三维有限元方法,模拟计算航空铝合金7050-T7451 材料在无内应力前提下数控铣削时产生的表层残余应力场。在综合考虑了现行的常规工艺方案基础上,从中选定4 种具有代表性的走刀路径分别进行分析计算,进而优选出最为合适的走刀工艺规则。走刀过程采用动态载荷步模拟,材料去除采用生死单元模拟,从而使计算结果更加精确、可信。通过本文的研究工作,可为提高该类材料数控铣削加工的尺寸稳定性确定合理的工艺策略。     

V型肋片直冷却通道内流动与传热的数值研究

采用结构化六面体网格和k-ε湍流模型求解三维N-S方程,对内置不同肋间距与肋高比V型扰流肋片的直冷却通道,在入口雷诺数为20 000时的流动与换热特性进行数值模拟,分析了不同肋间距与肋高比对肋间壁面换热效果和流动损失的影响,并对肋间距与肋高比进行了全局寻优。结果表明,带肋直冷却通道的整体换热效果和综合冷却效率,分别和肋间距与肋高比呈近似函数关系,肋间距与肋高比为7.93时通道整体换热效果最好,为5.2时通道综合冷却效率最佳。     

基于非线性试验气动力的飞机静气动弹性响应分析

分别使用线性和非线性静气动弹性分析方法,对某飞机纵向静气动弹性响应特性随飞行动压、攻角、平尾偏度和纵向过载变化的趋势进行了分析,并将分析结果和飞行试验进行了比较。线性方法的气动力计算使用亚音速偶极子格网法。非线性方法由风洞试验提供刚体气动力,并使用线性气动力影响系数矩阵对其进行弹性化处理。通过对两种方法的计算结果进行对比分析可以看出:①使用刚体试验气动力的非线性分析方法能够获得和飞行试验比较一致的结果;②在线性方法所提供的结果中,翼面的弯曲变形及剪力、弯矩和扭矩等部分参数能为初步设计提供大致参考,但气动力系数的弹性增量、翼面的扭转变形、翼面的剪力、弯矩和扭矩的弹性部分可能不能为型号设计提供正确的指导;③不论刚体气动力为线性还是非线性,气动力系数随动压变化的趋势均呈线性。     

基于有色载入技术的天基雷达信号处理方法

为了消除天基监视雷达非稳态杂波图景的影响,文中讨论一种利用有色载入（Colored-loading,CL）技术计算杂波协方差矩阵的空-时自适应处理（Space-time adaptive processing,STAP）方法。首先根据先前相干处理间隔（Coherent process interval,CPI）立体数据和先验知识,对杂波区域分块定位。并根据最大似然估计准则,估计各杂波块回波强度。对杂波回波强度进行归一化,并在多个CPI上取平均,得到杂波反射特性地图。结合该地图和先验知识,计算当前CPI的杂波协方差修正矩阵,将该修正矩阵有色载入当前CPI的杂波协方差矩阵,并对有色载入后的协方差矩阵进行主要特征值分析和重构。仿真结果表明,在天基雷达杂波环境中,该知识辅助CLSTAP算法远优于传统的滑窗处理（Sliding window processing,SWP）STAP算法性能,且与理想STAP算法的性能接近。     

从自由试验提取具有弹性支承的阻尼约束结构的主模态

作者已对边界固持(即刚性支承)的无阻尼和有阻尼的约束结构，从自由试验提取其实模态和主模态的方法进行过系统的研究，同时，对于具有弹性支承的无阻尼约束结构模态的提取，也建立了一种可行的方法。这些方法和技术途径都取得了良好的结果，仅剩下具有弹性支承的阻尼约束结构主模态的提取方法尚无。对此，本文企图建立一种工程中可行而实用的方法。在该方法中，阻尼分为瑞利阻尼和粘性阻尼两种模型，这样，可以根据不同结构选用不同阻尼模型下的提取方法。数值模拟结果表明，本文建立的方法虽然不像以前无阻尼下的类似方法那样，具有普遍性，即取任何支承刚度(可以很大或很小)都可获得满意结果。不过，对于工程中常见的支承刚度比结构刚度大或等量级的实际情况，本文方法是能取得满意结果的。这表明，本文方法已基本满足工程要求了。     

电机智能制造信息化平台

通过对电机制造工艺的分析,以及实地调研电机生产企业运行现状的基础上,针对电机制造工艺复杂、人工依赖大等特点提出了一种电机智能制造信息化平台建设方案。就整体信息系统提出了基于电机行业的工厂模型建立以及系统集成的建议,为电机行业建设智能制造工厂、优化生产管理提供参考。     

Deterministic pion and muon transport in Earth’s atmosphere

An accurate understanding of the physical interactions and transport of space radiation is important for safe and efficient space operations. Secondary particles produced by primary particle interactions with intervening materials are an important contribution to radiation risk. Pions are copiously produced in the nuclear interactions typical of space radiations and can therefore be an important contribution to radiation exposure. Charged pions decay almost exclusively to muons. As a consequence, muons must also be considered in space radiation exposure studies. In this work, the NASA space radiation transport code HZETRN has been extended to include the transport of charged pions and muons. The relevant transport equation, solution method, and implemented cross sections are reviewed. Muon production in the Earth’s upper atmosphere is then investigated, and comparisons with recent balloon flight measurements of differential muon flux are presented. Muon production from the updated version of HZETRN is found to match the experimental data well.     

Numerical simulations of the radiance from the comet 46P/Wirtanen in the various configurations of the measurements during “Rosetta” mission

The work we present deals with the spectrometric measurements of VIRTIS instrument of the Comet P/Wirtanen planned for the Rosetta mission. This spectrometer can monitor (VIRTIS M channel: 0.250μm – 0.980μm; Δκ=20cm⁻¹; 0.980 – 5.0 μm; Δκ = 5cm⁻¹; VIRTIS H channel: 2.0 μm – 5.0 μm; Δκ=2cm⁻¹) the nucleus and the coma in order to provide a general picture of coma's composition, the production of gas and dust, the relationship of coma production to surface composition and the structure and variation of mineralogy of the nucleus surface. During the mission the observation conditions of the spectroscopic investigation change due to different relative positions spacecraft/comet, and to the different illumination conditions of the surface at various distances of the comet to the Sun. The nucleus surface is continuously modified by the ice sublimation accompanied by gas and dust emission. Consequently the surface also its spectrophotometric properties changes and their monitoring can give a new insight. The important role of simulations is to predict the results of measurements in various experimental condition what, in the future, can help in interpretation of the measured data.

In this paper the first results of our simulation the radiance from the comet in the 0.25–5.0μm spectral range at two distances from the Sun (1AU and 3AU) are shown. The distance between the Rosetta orbiter and the nucleus surface as well as the sun zenith angles are taken into account according to the Rosetta mission phases. In fact the surface and coma properties vary along the comet orbit, and should be taken into account in our calculations. The optical parameters of the dust on the surface (e.g. reflectance) and in the coma (e.g. Q_ext) were calculated from optical constants of possible comet analogues. The thermodynamic parameters of the comet are taken from the models of comet evolution. Through this kind of modelling it is possible to identify the surface characteristics in spectra of the radiation from the surface of nucleus transmitted through the coma loaded with dust and gases.

Even if the “Rosetta mission” is postponed, with the consequence of a target change, we think that our idea and the method used for the simulations can be useful also for the new Rosetta target - the comet 67P/Churyumov Gerasimenko.     

混压式进气道与弹体一体化流场数值模拟

基于Favre平均的N－S方程和B／L代数湍流模型,采用Jameson格式和矩阵人工粘性,对X布局的混压式超声速进气道与弹体的一体化流场进行了数值模拟,研究了解决了数值计算中的附面层抽吸及混压式进气 启动问题,得出了进气道内外流场的马赫数分布和速度分布,讨论了绕弹体非均匀来流条件下,进气道的位置,附面层抽吸及攻角对进气道性能的影响和进气道外型形状对弹性气动力的影响,结果表明,对混压式进气道必须进行附面层抽吸,进气道的位置对进气道的性能有很大的影响,进气道的外型型面对弹体的气动性能有一定的影响。