同轴突扩燃烧室低频不稳定燃烧数值模拟

采用大涡模拟耦合预混燃烧方法,建立了液体冲压发动机不稳定燃烧计算模型。对模型发动机进行了不稳定燃烧数值研究,计算得到的发动机内压强振荡和火焰传播过程与文献中的实验数据吻合较好。结果分析表明,突扩构形发动机内大尺度的旋涡结构支配了燃烧室中的火焰传播过程,旋涡运动耦合非稳态的燃烧热释放是激发燃烧室低频压强振荡的重要原因。     

水反应金属燃料发动机初步试验

介绍了水反应金属燃料发动机试验系统,提出了水燃比、工作压强及试验燃烧效率计算方法,为试验设计和发动机性能评价提供了依据。对水反应金属燃料发动机进行了试验研究,并根据试验结果对药柱组分、发动机结构及供水系统进行了改进。试验表明,中等含量金属燃料加水后可稳定燃烧,通过增加燃料中镁含量、稳定进水流量和增加补燃室长度等措施,可有效提高发动机燃烧效率。     

Cosmic radiation exposure of aircraft occupants on simulated high-latitude flights during solar proton events from 1 January 1986 through 1 January 2008

From 1 January 1986 through 1 January 2008, GOES satellites recorded 170 solar proton events. For 169 of these events, we estimated effective and equivalent dose rates and doses of galactic cosmic radiation (GCR) and solar cosmic radiation (SCR), received by aircraft occupants on simulated high-latitude flights. Dose rate and dose estimates that follow are for altitudes 30, 40, 50, and 60 kft, in that order.     

A new modeling method of solar energetic proton events for ISO specification

Solar energetic protons degrade performance and reliability of spacecraft systems due to single-event effects, total dose effects and displacement damage in electronics components including solar cells. On designing a solar cell panel, a total fluence of solar energetic protons (SEPs) which cause solar cell damage is needed to estimate power loss of the solar cells over mission life. Nowadays a solar panel area of spacecraft is increasing as spacecraft mission life becomes longer (15–18 years). Thus an accurate SEP model is strongly required for the cost-minimum design from the aerospace industry. The SEP model, JPL-91 proposed by Feynman et al., is currently used widely for solar cell designing. However, it is known that the JPL-91 model predicts higher fluences of protons than values actually experienced in space, especially after 7 years on orbit. In addition, the model is based on several assumptions, and also needs Monte-Carlo simulations for calculating fluences. In this study, we propose a new method for modeling SEPs especially focused on solar cell degradation. The newly-proposed method is empirical, which constructs a model based directly upon proton flux measurement data taken by instruments onboard spacecraft. This method has neither assumptions nor dependence on SEP event selection, both of which are needed in JPL-91. The model fluences derived from this method show lower fluences in longer missions compared to JPL-91. This method has been proposed to ISO (International Organization for Standardization) and has been discussed for a new standard SEP model.     

鸟撞飞机风挡动态响应数值模拟方法研究现状

总结了目前用于鸟撞飞机风挡动态响应的数值模拟方法,主要有解耦解法、耦合解法和光滑质点动力学法,其中耦合解法涉及接触-碰撞耦合解法和流固耦合解法。各种方法围绕鸟体（鸟撞载荷）的模拟和风挡的模拟,部分内容针对鸟撞击发动机叶片、雷达罩和垂直尾翼等,但其方法同样适用于飞机风挡,最后指出应进一步深入研究的内容。     

基于改进支持向量机的油液在线监测系统

搭建油液在线监测实验平台进行磨粒分类识别实验,运用支持向量机和最近邻法相结合的方法对飞机发动机油液中的磨粒进行分类识别;其中基于支持向量机的磨粒分类器的输入为磨粒的主轴长度、纹理相关性、圆度等特征参数,输出为磨粒的分类结果;实验结果表明,基于支持向量机的磨粒分类器的分类准确率高达94％,并且由于最近邻法的使用,分类器的处理速度也提高了30％。     

FDTD-PML方法在柱形散射体总场计算中的应用

利用时域有限差分（FDTD）方法,结合理想匹配层（PML）吸收边界条件,对无限长柱形散射体的总场计算进行分析并得出数值解。证明了该方法在散射体总场计算中的实用性和有效性,并在此基础上给出了不同入射波源及PML参数对计算结果的影响。     

近红外光谱测定喷气燃料馏程的应用研究

以50个喷气燃料样品的近红外光谱数据和它们对应的化学测定数据为基础,对喷气燃料的馏程（初馏点,10%,20%,50%,90%）建立了校正模型。在所有的校正模型中,原始谱图经过二阶微分和偏最小二乘法（PLS）和完全交互验证法处理,校正模型的决定系数（R2）分别为0.808 7,0.796 5,0.693 6,0.649 9,0.740 4,校正集样本的标准偏差（SEC）分别为1.571,0.485,0.736,0.387,0.575。试验结果表明：该方法具有分析速度快、操作简单等特点。     

铷原子频标TE111微波腔的仿真分析及实验

使用AnsoftHFSS软件建立铷原子频标微波腔内加载集成泡的模型,仿真并分析了集成泡尺寸和安装位置对腔体谐振频率的影响,最后进行了实验验证。结果表明,仿真得出的结论和实验结果有一定的一致性,加载不同尺寸集成泡对微波腔谐振频率影响明显并且呈一定规律分布,这对于中微波腔的设计具有重要的参考价值。     

基于磁检测的AGV导引新方法

利用磁阻传感器作为磁导引路径的检测元件,实现了准确的磁路径定位,在此基础上实现了磁导引。详细介绍了磁检测方法、导引原理以及控制方案。当AGV产生一定范围的位置偏差时（水平偏移不大于±5cm,角度偏转不大于±25°）,该方法可以准确的检测并计算出位置偏差并进行相应控制。实验结果表明,该磁导引方式定位准确且易于实现。