高压软管脉冲试验设备

高压软管脉冲试验,是检测液压软管在制造过程中材质和接头压接质量的重要手段之一,从而保证飞机在进行各种科目飞行时,高压软管在高压脉冲下不破裂,不漏油。本文介绍一种结构简单、脉冲压力变化大、频率变化快,适合各种软管压力脉冲试验的新技术、新方法。     

菜园坝长江大桥主拱节段风洞试验及分析

中承式拱桥属于柔性空间结构,主拱上承受的脉动风荷载相互干扰。以重庆菜园坝长江大桥为研究对象,进行了湍流下的主拱单拱及双拱节段模型风洞试验。对模型表面脉动压力的功率谱、相关系数、水平和竖向相干函数进行了细致分析,讨论了双拱间距宽度比对脉动压力频域特性的影响。当间距宽度比大于5时,后拱风荷载受到前拱的干扰作用。当两拱间距宽度比小于5时,前后拱风荷载特性类似于组合截面。随间距宽度比变小,主拱涡脱落折算频率和压力功率谱逐渐增大,前后拱迎风面和背风面的相关系数及相干系数均逐步降低。     

气体减压阀的稳定性分析

针对逆向卸荷式气体减压阀,采用线性化分析方法,对其工作稳定性进行分析．得到了主要参数对减压阀稳定性的影响规律。研究结果表明阻尼和低压腔体积是影响减压阀稳定性的主要因素,并给出了提高减压阀稳定性设计的主要措施。     

航空发动机环形燃烧室噪声总声级的GMDH方法研究

采用数据处理的组合方法（GMDH）,研究航空发动机环形燃烧室测试数据。通过简单的二元二次回归原理来构造出下一代较为复杂的次级回归方程,并且利用＂优选原理＂淘汰掉次级回归方程中的那些不理想的项,得到燃烧室噪声总声级的高阶方程,获得较客观的描写复杂非线性系统的非线性模式。     

模压压力对焦炭颗粒增强沥青基炭复合材料性能的影响(英文)

采用普通液压机和新型高效的模压半炭化成型工艺,在大气环境下制备出了高密度、低成本的焦炭颗粒增强沥青基炭复合材料.研究了模压压力对焦炭颗粒增强沥青基炭复合材料的体积密度和抗压强度的影响趋势,并探讨了复合材料的体积密度与抗压强度之间的相互关系.结果表明,增大模压压力,沥青基炭复合材料的体积密度和抗压强度随之明显增加;继续增大模压压力,体积密度仍然呈上升趋势,但抗压强度却突然下降;沥青基炭复合材料的体积密度越高,其抗压强度未必也就越大.     

带导流叶排的轴流压气机级叶尖处理机匣容畸变特性

基于叶尖处理机匣轴流压气机叶排实验特性,应用畸变传递的矩阵分析模型,分析了进口导流叶排对叶尖处理机匣结构容总压畸变特性影响,初步建立了在进口导流叶排下几种处理机匣结构对总压畸变及其沿轴流压气机叶排衰减特性影响规律。计算结果表明,叶尖处理机匣虽均能有效提高压气机级的稳定工作范围,但削弱了转子叶排和静子叶排的抗总压畸变能力,这对设计合理的扩大轴流压气机稳定裕度处理机匣结构尤为重要。      

燃烧室柱部直径对脉动发动机工作特性的影响研究

建立了直接测量Helmholtz型脉动发动机燃烧室内气流压力的压力测试系统,应用该系统可实时监测发动机内气流脉动情况。研究了燃烧室柱部直径对燃烧室内气流压力波形、发动机的工作频率、燃油消耗率和过量空气系数等参数之间的影响关系。结论为在所研究的燃烧室柱部直径变化范围内,燃烧室柱部直径的变化对这些参数的影响并不明显,而油门开度对这些参数的影响却较大。      

气体静压轴颈-止推串接型轴承静特性的分析

采用有限元方法研究了狭缝节流气体静压轴颈-止推串接型轴承的静态特性,分析了节流狭缝宽度和气膜厚度等因素对径向和轴向承载性能的影响,研究了三棱形圆度误差对径向和轴向承载能力的影响, 揭示了轴颈轴承部分和止推轴承部分之间的相互影响规律,并且研究了当有误差存在时轴承内部气膜压力分布的规律。     

电推进系统压力调节单元的建模和分析

 建立了电推进系统压力调节单元的数学模型,利用Matlab/Simulink软件分析几个重要参数对系统的影响。仿真结果表明,采用bang-bang控制策略具有较高的控制精度,可满足系统的指标要求。     

Semi-analytical investigations of high area-to-mass ratio geosynchronous space debris including Earth’s shadowing effects

This paper investigates the long-term perturbations of the orbits of geosynchronous space debris influenced by direct radiation pressure including the Earth’s shadowing effects. For this purpose, we propose an extension of our homemade semi-analytical theory [Valk, S., Lemaître, A., Deleflie, F. Semi-analytical theory of mean orbital motion for geosynchronous space debris under gravitational influence. Adv. Space Res., submitted for publication], based on the method developed by Aksnes [Aksnes, K. Short-period and long-period perturbations of a spherical satellite due to direct solar radiation. Celest. Mech. Dyn. Astron. 13, 89–104, 1976] and generalized into a more convenient non-singular formalism. The perturbations accounting for the direct radiation pressure with the Earth’s shadow are computed on a revolution-by-revolution basis, retaining the original osculating Hamiltonian disturbing function. In this framework, we compute the non-singular mean longitude at shadow entry and shadow exit at every orbital revolution in opposition to classical approaches where the singular eccentric anomalies at shadow entry and shadow exit are computed. This new algorithm is developed using non-singular variables. Consequently, it is particularly suitable for both near-circular and near-equatorial orbits as well as orbits which transit periodically around null eccentricities and null inclinations.The algorithm is tested by means of numerical integrations of the equations, averaged over the short periods, including radiation pressure, J₂, the combined Moon and Sun third body attraction as well as the long-term effects of the 1:1 resonance occurring for geosynchronous objects. As an extension of [Valk, S., Lemaître, A., Anselmo, L. Analytical and semi-analytical investigations of geosynchronous space debris with high area-to-mass ratios influenced by solar radiation pressure. Adv. Space Res., doi:10.1016/j.asr.2007.10.025, 2007b], we especially apply our analysis to space debris with area-to-mass as high as 20 m²/kg. This paper provides numerical and semi-analytical investigations leading to a deep understanding of the long-term evolution of the semi-major axis. Finally, these semi-analytical investigations are compared with accurate numerical integrations of the osculating equations of motion over time scales as high as 25 years.