内并联型TBCC进气道方案设计及验证

提出了一种带可变几何泄流腔的内并联型涡轮基组合循环(TBCC)进气道设计方案.介绍了进气道的总体设计思路,给出了进气道的设计马赫数、转级马赫数及飞行轨迹,对不同来流条件下进气道的工作方式以及全马赫数范围进气道型面调整的安排进行了论述,确定了进气道主要气动参数与型面参数的选取原则.通过数值模拟和高速风洞试验的手段,对进气道设计方案的可行性进行了验证.数值模拟结果表明:当Ma₀≤2.5时,进气道的总压恢复系数均在0.8以上,当2.5<Ma₀≤4.5时,进气道的总压恢复系数均在0.3以上,符合进气道总体方案的要求;冲压模态下,冲压通道的出口马赫数均小于0.4,出口静压均大于0.5个标准大气压,均能满足冲压燃烧室的燃烧需求.风洞试验结果表明:模态转换过程中,进气道涡轮通道具有良好的进/发匹配特性,且进气道涡轮/冲压通道具有良好的相容性能.研究结果可为我国开展组合动力研究提供方案参考和技术储备.      

基于T96模型的极尖区位形变化特性研究

基于T96模型,定义了极尖区的位形以及相关的描述参量(例如赤道向边界磁纬的最小值,纬向宽度,子午向和晨昏向的张角,倾斜度,扁平度,中心磁地方时等),讨论了太阳风动压(P_d)、行星际磁场(IMF)及磁暴强度对极尖区位形的影响.太阳风动压和磁暴强度越大,则极尖区的赤道向边界磁纬越小,纬向宽度越大,子午向和晨昏向的张角越大,倾斜度越大,扁平度越小;南向IMF B_z越强,则极尖区的赤道向边界磁纬越小,纬向宽度越小,子午向的张角越小,晨昏向的张角越大,倾斜度越大,扁平度越大;北向IMF B_z与南向IMF B_z的情况刚好相反;极尖区的中心磁地方时受IMF B_y控制,IMF B_y为正时,极尖区向昏侧移动,而IMF B_y为负时,极尖区则向晨侧移动,并且极尖区的中心磁地方时与IMF B_y之间有着良好的线性关系.将所得结果与前人的观测结果进行了简单比较,发现利用T96模型确定的极尖区位形与观测基本一致.     

动力舱冷却用排气引射混合管改进设计方法

对直升机动力舱冷却用的排气引射混合管的设计方法进行了研究,基于引射器特性方程和对引射特性影响因素的分析,参考某型直升机发动机排气系统,提出了针对直升机动力舱冷却用的排气引射混合管设计的改进方法——修正系数法.应用该方法,针对某型发动机动力舱冷却用排气引射混合管进行了设计,并与实验结果进行了对比,结果表明,该方法可以使设计效率提高30%,设计精度保持在5%以内,满足工程设计要求,具有工程应用价值.      

一种适用于进近尾流间隔缩减的机型聚类方法

目前,我国广泛使用的尾流间隔标准过于保守,导致机场跑道容量受限。以进近航空器的尾流遭遇问题为研究对象,首先研究进近尾流安全间隔缩减方法,获取缩减后的临界尾流间隔;然后基于主成分分析法（PCA）对 BADA 数据库中的航空器性能数据降维,提出一种适用于进近尾流间隔缩减的机型层次聚类方法;最后采用该方法得到新的机型分类结果并构建缩减后的尾流安全间隔标准。结果表明：本文所使用的机型层次聚类方法与国内外航空器分类方法具有较好的一致性,在长沙黄花国际机场的主流配对机型间,所获取的进近航空器尾流间隔标准与传统尾流间隔标准相比可以缩减 0.8 km 以上。     

基于Origin语言的某型教练机发动机燃油系统故障诊断与分析

某型教练机在低空大表速飞行时,其发动机在最大状态下的供油量超过了发动机在各个状态的最大燃油流量软件值（GT=2300kg／h）,发动机从主燃油流量控制转为发动机应急流燃油量控制。本文对发动机色行数据进行了深入分析,同时结合发动机的三大特性,对其控制系统软件进行更改,经过后续飞行验证．发动机燃油控制系统下作正常。     

The effect of the space flight environment on mucin production in the mouse uterine tube

Numerous studies have indicated that the microgravity environment of space has harmful effects on several tissues throughout the body. Although this phenomenon is well documented, research in this area is still in its relative infancy. This study investigates the effects of space flight on mucin production of the uterine tubes of mice. This study examined the epithelium of the uterine tubes from female mice that were flown on the space shuttle Endeavour for 13 days in August, 2007 and their concomitant controls. The tissue was qualitatively analyzed for the type of mucin produced, i.e., acidic, neutral, acidic/neutral mixture. Further, the tissue was quantitatively analyzed for the amounts of mucins produced by measuring the thickness of the mucin layer for each region of the uterine tube: isthmus, ampulla, and infundibulum. One way ANOVA tests were used to compare mucin thickness between all three sets of animals. Results indicate similar but not identical results between the three regions of the uterine tube. The Baseline tissue had the thickest mucin layer regardless of treatment group. In the ampulla the mucin layer was the thinnest in the Flight tissue, followed by the Ground Control, with the Baseline being the thickest. Analysis of the mucin layer of the infundibulum of the three treatment groups indicated no difference in its thickness between the three regions of the uterine tube. These results indicate a trend toward thinning of the mucin layer of the uterine tube in space flight, but also indicate an influence by the housing environment.     

叶片模态分析的单元类型选择

由于有限元单元类型的选择、网格划分精细程度上的不同,同一个模型的分析结果会有不同。本论文结合某型航空发动机叶片模态分析的实例,分析了单元类型的选择和网格划分精细程度的高低对分析结果精度的影响;揭示了随网格划分精细程度的变化,分析结果的收敛规律;并用有理论解的悬臂梁验证了收敛规律。     

甲烷-空气贫燃料预混燃烧的数值模拟

针对燃气轮机燃烧室火焰筒中的甲烷-空气贫燃料预混燃烧问题,给出了基于八步化学反应动力学机理的数学模型。以某型航空发动机燃烧室火焰筒为例,对甲烷-空气贫燃料的预混燃烧进行数值模拟。研究结果表明,基于八步化学反应动力学机理的数值模拟方法,可以比较准确地反映燃烧产物的形成过程,在分析航空发动机燃烧室火焰筒内的贫燃料预混燃烧问题时具有较强的实用性。     

带旋流器的燃油喷嘴工作特性及火焰筒头部数值模拟

对带空气旋流器的燃油喷嘴工作特性进行了试验研究,得到了该喷嘴的供油特性、喷雾锥角的变化特点和液滴尺寸及其分布规律。应用Fluent软件模拟了在最大工作状态下火焰筒头部和喷嘴喷雾的相互作用,重点计算了火焰筒头部的空气流场、浓度场和油滴轨迹。通过喷嘴试验和数值模拟,真实地反映火焰筒头部的物理化学过程,为该喷嘴和火焰筒的改进提供了重要依据。     

Characteristics of field line resonance type geomagnetic pulsations and variations of plasmaspheric plasma density distribution

The period of field line resonance (FLR) type geomagnetic pulsations depends on the length of the field line and on the plasma density in the inner magnetosphere (plasmasphere), where field lines are closed. Here as FLR period, the period belonging to the maximum occurrence frequency of the occurrence frequency spectrum (equivalent resonance curve) of pulsations has been considered. The resonance system may be replaced by an equivalent resonant circuit. The plasma density would correspond to the ohmic load. The plasma in the plasmasphere originates from the ionosphere, thus FLR period, occurrence frequency are also affected by the maximum electron density in the ionosphere. The FLR period has shown an enhancement with increasing F region electron density, while the occurrence frequency indicated diminishing trend (possible damping effect). Thus, the increased plasma density may be the cause of the decreased occurrence of FLR type pulsations in the winter months of solar activity maximum years (winter anomaly).