弹性悬挂弯扭耦合颤振模型表面压力分布的时空特性及颤振机理分析

实际应用中,桥梁颤振稳定性可用风洞试验的结果作为评估标准,但颤振时断面的压力空间分布特征是不清楚的。本文对弹性悬挂的刚体模型在颤振时及固定时(来流风速与颤振风速一致)的表面压力进行采样,首先分析模型在颤振时的表面各部分压力特性,结果显示,右部压力相位相当于左部具有滞后性,表明是受迎风侧特征紊流影响的被动区域。随后运用本征正交分解(POD)方法分析模型表面压力分布特征与颤振发散性运动之间的关系,结果显示,所获得的本征模态中存在与颤振扭转发散运动关联极强的'主导颤振模态',该模态对总升力矩系数波动的贡献占绝对主导地位,其主坐标频率与颤振频率一致且具有与振动位移一致的发散性,但其归一化空间分布特征在断面颤振过程中不变化。结合模型在固定时的本征模态分析结果,除颤振主导模态外,其余模态均能在固定时的本征模态中找到类似空间分布的模态,且与断面发散性运动的关联性很小。本文工作为今后颤振机理分析提供了一个新的思路与方法。     

一种用于空间翻滚目标接近控制的相对运动建模方法

针对空间翻滚目标等一类相对运动复杂的接近控制问题,首先重点研究了基于微分几何理论的相对运动建模,建立视线旋转坐标系下的三维相对运动方程;然后将三维相对运动解耦为视线瞬时旋转平面内的相对运动和该平面的转动,建立了统一的控制器设计框架,形式统一简洁、物理意义明确,消除传统制导与控制策略中俯仰、偏航通道的耦合因素影响;最后通过六自由度仿真算例证明,相对运动模型物理意义明晰、鲁棒性强、控制精度高、工程实现容易。     

December 2006 solar extreme events and their influence on the near-Earth space environment: “Universitetskiy-Tatiana” satellite observations

The Russian microsatellite “Universitetskiy-Tatiana” was launched on Jan. 20, 2005 and was both a scientific and educational mission. Its two main aims were declared as: (1) monitoring of the energetic particles dynamics in the near-Earth space environment after solar events and during quiet times, (2) educational activities based on experimental data obtained from the spacecraft. In this paper observations acquired during Dec. 5–16, 2006, known as “Solar Extreme Events 2006”, were analyzed. The “Universitetskiy-Tatiana” microsatellite orbit permits one to measure both solar energetic particle dynamics, variations of the boundary of solar particle penetration, as well as relativistic and sub-relativistic electrons of the Earth’s outer radiation belt during and after magnetic storms. Both relativistic electrons of the Earth’s outer radiation and solar energetic particles are an important source of radiation damage in near-Earth space. Therefore, the presented experimental results demonstrate the successful application of a small educational spacecraft both for scientific and educational programs.     

大口径蝶阀数学建模与流场特性分析

为了获得大口径蝶阀的输入输出特性模型,开展了蝶阀运动特性实验和数值模拟仿真研究。在给定工况下,计算蝶阀在不同开度下的速度、压力、力矩和压降,获取了蝶阀内部流场特性;同时,根据流速分布、压力分布、湍流动能和湍流强度等表征蝶阀流动特性的参数,通过拟合建立了蝶阀特性数学模型,并与实验数据进行了 对比分析。结果表明:不同开度时,蝶阀呈现不同的流场特性,当开度大于等于5365%时,蝶阀流体在入口和出口处的流速较饱满,流通性能相对较好,流态平稳。经实验数据修正后的蝶阀数学模型置信度高,利用它进行蝶阀运动特性数值模拟分析是可行性的。     

Observational constraints on dark matter in the universe

Application of the cosmic virial theorem to galaxy redshift surveys suggests an open universe - if the dark material is distributed in the same way as galaxies. Here we investigate four redshift surveys. We present new results on the amplitudes of the two- and three-point galaxy correlation functions and we estimate the relative peculiar velocities in the deep redshift survey of Kirshner and co-workers (1983). Next, we review evidence which suggests that dark material is clustered on scales comparable to the optical radii of galaxies. In particular, we use spectroscopic and photometric observations to set constraints on the mass distribution in elliptical galaxies.     

高分辨率卫星遥感图像的偏流角及其补偿研究

卫星遥感采用高分辨率TDICCD相机时，由于地球的旋转产生图像运动的偏流角，偏流角对这种遥感图像的质量影响较大，需要进行补偿，并通过遥感视线的校正实现。补偿的首要工作是确定图像运动的偏流角和遥感视线的修正量。基于航天器飞行动力学原理，本文求出了各种近地轨道的偏流角、偏流角角速度，把遥感视线的校正分成粗校正和精校正，并给出了修正量的确定方法。针对椭圆轨道和圆轨道情况的偏流角及修正量的计算，验证了本文算法的有效性。     

Multi-case Study of Current Sheet Flapping Motions Induced by Non-adiabatic Ions

In this paper, the y-component of magnetic field line curvature in the plasma sheet was analyzed, and two kinds of shear structures of the flapping current sheet were found, i.e. symmetric and antisymmetric. The alternating bending orientations of the guiding field are exactly corresponding to alternating north-south asymmetries of the bouncing ion population in the sheet center. Those alternating asymmetric plasma sources consequently induce the current sheet flapping motion as a driver. In addition, a substantial particle population with downward motion was observed in the center of a bifurcated current sheet. This population is identified as the quasi-adiabatic particles, and provides a net current opposite to the conventional cross-tail current.     

尾缘吹气式稳定器后体角对燃烧性能影响的试验

通过数值模拟了后体角为60°,120°和180°三种尾缘吹气稳定器的回流区,试验测试了后两种稳定器的冷态雾化场、贫熄边界和燃烧效率,从而研究了尾缘后体角改变对其燃烧性能的影响.试验结果表明由于后体角直接影响回流区大小和雾化质量,从而影响稳定器的燃烧性能.燃烧试验表明120°尾缘吹气稳定器贫熄边界和燃烧效率优于后体角为180°的稳定器和槽宽大50%的V型稳定器.      

Long term and safe relative orbit design for heterogeneous spacecraft clusters

The problem of obtaining long term relative orbit configurations for spacecraft clusters with realistic operational considerations such as safety, station keeping and inter-spacecraft distances is addressed. Two different approaches are developed for station keeping and safety objectives. In the first approach, relative orbit configurations, or relative TLEs, are found minimizing deviations from reference mean orbit which would maximize the station-keeping objective. In second one, relative configurations are found from a reference initial condition by minimizing probability of collision, hence maximizing the safety objective, between the spacecraft in the cluster which are propagated numerically through a high precision orbit propagator. For the design optimization, a derivative free algorithm is proposed. Effectiveness of the approaches is demonstrated through simulations. Using this design framework, several configurations can be found by exploring the limits of the clusters in terms of spacecraft number, distance bounds and probabilities of collision for long time intervals.     

三维试验粒子轨道法在磁层粒子全球输运中的应用

根据磁层粒子动力学理论, 通过偶极磁场模型验证利用三维试验粒子轨道方法模拟近地球区(r < 8R_e)带电粒子运动特征的可靠性. 在此基础上, 以太阳风和磁层相互作用的全球MHD模拟结果为背景, 利用三维试验粒子轨道方法, 对非磁暴期间南向行星际磁场背景下太阳风离子注入磁层的情形进行数值模拟, 并对北向行星际磁场背景下太阳风离子注入极尖区以及内磁层的几种不同情形进行了单粒子模拟. 模拟结果反映了南向和北向行星际磁场离子向磁层的几种典型输入过程, 揭示出行星际磁场南向时太阳风粒子在磁层内密度分布的晨昏不对称性以及其在磁鞘和磁层内的大致分布, 并得出统计规律. 模拟结果与理论预测和观测结论相一致, 且通过数值模拟发现, 行星际磁场北向时靠近极尖区附近形成的非典型磁镜结构对于能量粒子经由极尖区注入环电流区域过程有重要的影响和作用.