液压阻尼器对模型旋翼地面共振的影响

 分析了某采用定压阀和补油装置的液压阻尼器的非线性特性。对无铰式模型旋翼的地面共振稳定性进行了数值仿真研究,分析了两种不同的非线性液压阻尼器对地面共振稳定性的影响。结果表明：由于补油分配阀间隙的影响,阻尼器低速时的有效阻尼大大下降;在无阻尼器的模型旋翼稳定的转速区内,该阻尼器不能改善系统小扰动情况时的动稳定性;在无阻尼器的模型旋翼不稳定区内,系统将出现极限环,且极限环幅值随补油分配阀间隙的增大而增大。研究结果对液压阻尼器的设计具有参考价值。     

燃烧室电火花点火模型

为了准确掌握影响航空发动机燃烧室点火边界的关键因素,并建立燃烧室点火边界预测模型,对单头部燃烧室的点火过程及点火边界进行了试验与理论研究。获取了燃烧室点火过程的火核生成与传播特性曲线,形成了拓宽燃烧室点火边界的优化方法,基于点火恢复时间建立了燃烧室点火边界预测模型,并对预测模型的精度进行验证。结果表明:提高喷嘴雾化性能是提升点火性能的最有效途径,点火模型预测结果与试验结果相符度较好,模型的最大误差小于20%,满足燃烧室工程设计需要。      

基于恒应变率控制的椭圆凹模胀形试验方法

为确定2A16-O铝合金板材在不同温度及应变率下的成形极限曲线(FLCs),应用改进Hollomon公式获取满足外插可靠度的拟合应力应变,通过有限元分析(FEA)不同椭圆度的椭圆凹模胀形破裂位置,优化工艺参数得到指定应变路径下的成形极限点,建立了液体压力与等效应变及应变率的公式,推导出压力变化率与应变率的定量关系。以应变率控制的椭圆凹模胀形与单拉试验相结合,获得2A16-O铝合金板材在不同温度及应变率下的FLCs,为定量分析应变率的影响规律和评判理论预测方法的准确性提供了依据。      

基于概率极限状态的RAIM风险评估

为了提供准确可靠的完好性服务,提出了基于概率极限状态的RAIM完好性风险评估。考虑所需导航性能参数和噪声的因素,建立了安全系数与可靠系数相结合的完好性风险评估指标体系,确立风险评价准则。非精密进近的算例分析表明,系统评估方法是可行的且有效的。     

Heliotropic dust rings for Earth climate engineering

This paper examines the concept of a Sun-pointing elliptical Earth ring comprised of dust grains to offset global warming. A new family of non-Keplerian periodic orbits, under the effects of solar radiation pressure and the Earth’s J₂ oblateness perturbation, is used to increase the lifetime of the passive cloud of particles and, thus, increase the efficiency of this geoengineering strategy. An analytical model is used to predict the orbit evolution of the dust ring due to solar-radiation pressure and the J₂ effect. The attenuation of the solar radiation can then be calculated from the ring model. In comparison to circular orbits, eccentric orbits yield a more stable environment for small grain sizes and therefore achieve higher efficiencies when the orbit decay of the material is considered. Moreover, the novel orbital dynamics experienced by high area-to-mass ratio objects, influenced by solar radiation pressure and the J₂ effect, ensure the ring will maintain a permanent heliotropic shape, with dust spending the largest portion of time on the Sun facing side of the orbit. It is envisaged that small dust grains can be released from a circular generator orbit with an initial impulse to enter an eccentric orbit with Sun-facing apogee. Finally, a lowest estimate of 1 × 10¹² kg of material is computed as the total mass required to offset the effects of global warming.     

On the effect of considering more realistic particle shape and mass parameters in MMOD risk assessments

One of the primary mission risks tracked in the development of all spacecraft is that due to micro-meteoroids and orbital debris (MMOD). Both types of particles, especially those larger than 0.1 mm in diameter, contain sufficient kinetic energy due to their combined mass and velocities to cause serious damage to crew members and spacecraft. The process used to assess MMOD risk consists of three elements: environment, damage prediction, and damage tolerance. Orbital debris risk assessments for the Orion vehicle, as well as the Shuttle, Space Station and other satellites use ballistic limit equations (BLEs) that have been developed using high speed impact test data and results from numerical simulations that have used spherical projectiles. However, spheres are not expected to be a common shape for orbital debris; rather, orbital debris fragments might be better represented by other regular or irregular solids. In this paper we examine the general construction of NASA’s current orbital debris (OD) model, explore the potential variations in orbital debris mass and shape that are possible when using particle characteristic length to define particle size (instead of assuming spherical particles), and, considering specifically the Orion vehicle, perform an orbital debris risk sensitivity study taking into account variations in particle mass and shape as noted above. While the results of the work performed for this study are preliminary, they do show that continuing to use aluminum spheres in spacecraft risk assessments could result in an over-design of its MMOD protection systems. In such a case, the spacecraft could be heavier than needed, could cost more than needed, and could cost more to put into orbit than needed. The results obtained in this study also show the need to incorporate effects of mass and shape in mission risk assessment prior to first flight of any spacecraft as well as the need to continue to develop/refine BLEs so that they more accurately reflect the shape and material density variations inherent to the actual debris environment.     

采用双模压缩态的光子纠缠光纤陀螺仪研究CSCD

对采用双模压缩态的光子纠缠光纤陀螺仪进行了理论研究,采用角动量理论首次推导了双模压缩态输入的光子纠缠光纤陀螺仪的相位检测灵敏度,并证明了当光子数足够大时,可以达到海森堡极限。针对采用双模压缩态的光子纠缠光纤陀螺仪的二阶符合计数探测方案远未达到海森堡极限的情况,通过考察光子纠缠光纤陀螺仪各输出态的二阶符合计数对总的二阶相关光强的贡献,发现二阶符合计数探测方案存在量子增强信息的抵消,也即其中一个接收端光子数为偶数的输出态和光子数为奇数的输出态的二阶符合计数形成互补的倍频干涉条纹,进而相互抵消。因此,需要优化探测方案,提取完整的量子增强信息,才能实现海森堡极限的相位检测灵敏度。     

超椭球凸集合可靠性综合指标定义及求解方法

针对失效域与超椭球凸集合发生干涉与不发生干涉两种情况下,超椭球凸集合非概率可靠性与非概率可靠度两种指标各自存在的不足,将两指标相结合提出多个超椭球凸集合描述时的可靠性综合指标定义,并提出将改进的有限步长迭代法(MLSA)与Monte-Carlo法结合来求解综合指标的方法.MLSA是在有限步长迭代法的基础上提出的,根据增...     

地面系留对直升机动力响应的影响

 建立了系留状态下直升机旋翼/机体耦合非线性动力学模型,无铰旋翼简化为当量铰刚性桨叶模型,假定机体是刚性体并受起落架和系留索的约束,系留索静态时松弛并只能承受拉力。采用数值仿真研究了系留对模型旋翼地面共振的影响,对初始扰动和旋翼转速对系统动力学行为的影响也进行了仿真研究。对于无系留的模型旋翼来说,在任何转速下没有出现不稳定现象;地面系留时系统会呈现稳定响应、极限环以及大幅值振荡等非线性动力学行为,大幅值振荡将使系留索、接头和支持结构承受破坏性动力载荷。     

直升机尾桨涡环飞行试验研究

根据样机右侧飞的飞行试验,对尾桨涡环现象进行了计算分析;根据右侧飞试验结果,估算出样机悬停回转时尾桨处于涡环状态的偏航角速度范围;将试验结果与国内外的涡环状态判据进行了对比。结果表明,国外的涡环判据不适用于样机的尾桨涡环状态判定,国内的高-辛判据与试验结果一致。