PIV 技术测量振荡射流流场

利用以大功率双脉冲激光器为光源的ＰＩＶ技术，测定了由扁平射流和尖劈组成的二维振荡射流流场。实验结果表明，射流喷嘴与尖劈之间存在交错的、旋转方向相反的涡街，从而在尖劈两侧形成压力扰动。这种压力扰动波与不稳定射流的相互作用是整个系统产生流体振荡的原因。此外，还分析了射流喷嘴与尖劈之间的距离对流场的影响规律。     

自由飞行下基于IPS算法的碰撞风险研究

自由飞行是解决空域拥挤问题的一种有效飞行模式。随着通信、导航、监视（ CNS ）技术的不断进步和自由飞行理论的不断完善,自由飞行将会使飞机由被动指挥向自选最优路径转变,能够明显提高空域的容量和飞行的效率。在评估自由飞行环境下飞机运行的安全性时,需要行之有效的碰撞风险评估方法。首先考虑通信、导航、监视（CNS）性能对飞机定位误差的影响,在执行飞行冲突解脱命令过程中引入相互作用粒子系统（IPS）,提出一种自由飞行下飞机碰撞风险评估算法,最后结合目标安全水平寻找最优最小安全间距。算例表明,算法能够快速有效计算自由飞行下飞机间碰撞风险,具有可行性。     

The effect of the longitudinal propagating waves on the electron acceleration in the reconnecting current sheet

Based upon the most efficient electron acceleration near the midplane of 3D non-neutral driven reconnecting current sheet (RCS) and the electrostatic wave excitation by the drift Maxwellian distribution of electrons in Vlasov simulation, we assume that the electrostatic waves mainly propagate opposite to the reconnecting electric field and investigated how these waves affect the electron acceleration. The main results are: (1) when the electron’s velocity equals to the phase speed of the waves, they will be trapped and have the different accelerating characteristics from the untrapped electrons through solving the momentum equations of electrons analytically; (2) the test particle simulations further prove that the number of the energetic electrons decreases with the increasing intensity of unstable waves, and the distribution of the energetic electrons takes on the double power-law.     

Aerodynamic multi-objective integrated optimization based on principal component analysis

Based on improved multi-objective particle swarm optimization (MOPSO) algorithm with principal component analysis (PCA) methodology,an efficient high-dimension multiobjective optimization method is proposed,which,as the purpose of this paper,aims to improve the convergence of Pareto front in multi-objective optimization design.The mathematical efficiency,the physical reasonableness and the reliability in dealing with redundant objectives of PCA are verified by typical DTLZ5 test function and multi-objective correlation analysis of supercritical airfoil,and the proposed method is integrated into aircraft multi-disciplinary design (AMDEsign) platform,which contains aerodynamics,stealth and structure weight analysis and optimization module.Then the proposed method is used for the multi-point integrated aerodynamic optimization of a wide-body passenger aircraft,in which the redundant objectives identified by PCA are transformed to optimization constraints,and several design methods are compared.The design results illustrate that the strategy used in this paper is sufficient and multi-point design requirements of the passenger aircraft are reached.The visualization level of non-dominant Pareto set is improved by effectively reducing the dimension without losing the primary feature of the problem.     

用非线性k-ε-k_p两相湍流模型模拟旋流两相流动

建立了两相湍流的代数应力模型 ,并由此出发 ,导出非线性k ε kp 两相湍流模型 ,目的是合理地模拟各向异性较强的旋流两相流动 ,保持二阶矩模型的优点 ,同时比二阶矩模型简单 .文中得到了气相、颗粒相的雷诺应力和两相脉动速度关联的非线性应力应变关系式。这些代数式和两相各自的湍动能k ,kp,以及两相脉动关联湍动能kpg的方程联立 ,就构成非线性k ε kp 模型 .将该模型用于模拟旋流两相流动 ,给出两相时均速度场及雷诺应力各分量 ,并且将模拟结果和实验数据以及二阶矩模型的模拟结果对照 .研究结果表明 ,该模型预报旋流两相流动的能力和二阶矩模型的能力相差不多 ,但计算量比二阶矩模型的小     

某型航空发动机燃油喷嘴的试验研究

本文对某型航空发动机燃油喷嘴的工作特性和雾化质量进行了试验研究。主要包括：测定喷嘴的流量特性，通过数码照相和计算机图像处理测定喷嘴在不同压力下的喷雾锥角，利用相位多普勒粒子分析仪（PDPA）和激光多普勒测速仪（LDV）测量喷嘴的雾化粒度SMD及尺寸分布。通过对上述试验结果的分析，得出了一些有价值的结论。这些结论对该发动机燃油喷嘴的改进提供了重要依据。     

熔铝氧化渗透合成SiC_p/Al_2O_3-Al复合材料的微观结构分析

以低成本的熔铝氧化渗透合成新方法制备了SiCp/Al2 O3 Al复合材料。借助X光电子谱 (XPS)、光学金相显微镜、透射电镜 (TEM)、X射线衍射 (XRD)等手段研究了该种复合材料的微观结构 ,并分析了影响微观结构的主要因素及其影响规律。结果表明 ,Al2 O3 和Al作为复合材料基体呈双连续分布 ,它们各自的含量可在较大范围内受SiC颗粒的粒度所控制。在熔铝氧化渗透合成的SiCp/Al2 O3 Al复合材料中 ,各组成相之间无界面反应 ,也无晶间相 ,Al2 O3 在SiC颗粒表面二次形核并直接生长的现象普遍存在 ,并由此形成了具有良好物理冶金结合的Al2 O3 SiC一体化陶瓷骨架     

The Marginal Rao-Blackwellized Particle Filter for Mixed Linear/Nonlinear State Space Models

In this paper, the marginal Rao-Blackwellized particle filter （MRBPF）, which fuses the Rao-Blackwellized particle filter （RBPF） algorithm and the marginal particle filter （MPF） algorithm, is presented. The state space is divided into linear and non-linear parts, which can be estimated separately by the MPF and the optional Kalman filter. Through simulation in the terrain aided navigation （TAN） domain, it is demonstrated that, compared with the RBPF, the root mean square errors （RMSE） and the error variance of the nonlinear state estimations by the proposed MRBPF are respectively reduced by 29% and 96%, while the unique particle count is increased by 80%. It is also found that the MRBPF has better convergence properties, and analysis has shown that the existing RBPF is nothing more than a special case of the MRBPF.     

3He-Rich Solar Energetic Particle Events

³He-rich solar energetic particle (SEP) events show huge enrichments of ³He and association with kilovolt electrons and Type-III radio bursts. Observations from a new generation of high resolution instruments launched on the Wind, ACE, Yohkoh, SOHO, TRACE, and RHESSI spacecraft have revealed many new properties of these events: the particle energy spectra are found to be either power-law or curved in shape, with the ³He spectrum often being distinctly different from other species. Ultra-heavy nuclei up to >200 amu are found to be routinely present at average enrichments of >200 times solar-system abundances. The high ionization states previously observed near ∼1 MeV/nucleon have been found to decrease towards normal solar coronal values in these events. The source regions have been identified for many events, and are associated with X-ray jets and EUV flares that are associated with magnetic reconnection sites near active regions. This paper reviews the current experimental picture and theoretical models, with emphasis on the new insights found in the last few years.     

Imaging diagnostics of solar non-thermal particles

Non-thermal hard X-ray, gamma-ray and radio emission are the most direct signatures of the presence of energetic particles in the solar atmosphere. This paper lays emphasis on hard X-ray and radio imaging data, obtained during and outside flares, which reveal the sites where particles interact with the ambient medium. These observations, which provide more or less direct information on the topology and dynamics of the magnetic structures in which particles are accelerated and propagate, are discussed in the framework of the statistical flare scenario.