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     

非线性分离算法及其在飞行试验中的应用

 本文根据最小方差估计和分离算法原理,提出一种新的非线性状态估计和偏差辨识的分离算法。并用此算法确定飞行状态和测试仪器的误差,同时U-D分解保证计算效率和数值稳定性。为了得到数据相容性检验的准确结果,本文采用直接离散化的飞机运动模型,以减小模型误差。通过仿真并在我国两种歼击机上实际应用,结果表明本文所给的算法对不同的初值和噪声统计特性都能得到飞行数据相容性检验的一致结果,并能用于低采样率下的数据相容性检验。     

基于模态滤波器改进的动载荷识别模型

 基于模态滤波器概念提出了对载荷识别模态模型法的原理性校正方案,构造了动载荷识别的离散模态滤波器模型。以其他点激励代替常常不可达的实际工作输入点,通过建立系统的模态参数并相继在模态和物理坐标下的求解对动态载荷作出估算,可以避免经典模态模型法通常对结构或边界条件所作的修改和由于模态参数自身误差而导致的较大识别误差,实例分析表明该模型识别精度较高并具有普遍的工程适用性。     

飞机大攻角空间机动气动力建模研究

 准确的气动力模型是大攻角机动仿真与控制等飞行动力学问题研究的基础。针对纵向运动建立的非线性非定常气动力微分方程模型扩展应用于一般空间运动形式,在分析大攻角非定常流动机理和试验数据的基础上,发展了一种多自由度非线性非定常气动力数学模型,并探讨了模型辨识和参数估计问题。用全机构形的大攻角动态风洞试验数据对模型进行的验证表明所发展的气动力模型能够描述大攻角气动力主要的非线性和非定常特性。     

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。     

飞控-飞机低阶等效系统的在线辨识

以飞控—飞机低阶等效系统为背景，采用Taylor展开法研究了带纯延迟环节的二阶系统的在线辨识。采取了对低信息点进行抛弃，变步数起动等算法对传统的最小二乘法加以改进，大大减少了辨识过程中产生的误差，更适合于实时辨识。实际应用结果表明：该方法可以有效地对具有时变特性的带纯延迟的非线性系统加以辨识，辨识结果满足工程要求。     

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.