两端固定输流管道在脉动内流作用下参数共振的最优控制

采用压电片作为控制执行元件,对两端固定输流管道在脉动流作用下的参数共振进行了最优控制.基于二次型性能指标最优控制原理,针对离散后的运动方程在零平衡点附近Jacobian矩阵的非时变部分设计了最优控制器.最后,通过数值仿真的方法对控制方案的有效性进行了验证.结果表明,该方案对输流管道在第一、第二振型次谐波共振区域及组合共振区域的参数共振的控制均有很好的效果.     

航天器弹性附件伸展动力学研究

利用动量矩定理推导出带伸展弹性板航天器的姿态动力学方程，在弹性板等速伸展的情况下，导出板的振动与伸展运动耦合微分方程，航天器姿态运动与板的伸展运动、振动耦合微分方程，通过龙格－库搭积分法得出了数值解，结果表明：弹性板等速伸展时，其振动的振幅随板长度的增长而增大，航天器姿态角速度随板长度的增长而减少。弹性板等速率越大，板振动的振幅越大。     

LU—ADI方法在求解跨声速翼型绕流问题中的应用

本文利用LU-ADI方法求解了跨声速范围内的Euler、NS方程。研究了边界的处理和某些求解方法的改进。     

The Changing Face of Titan’s Haze: Is it all Dynamics?

Titan’ atmosphere shows some similarities with that of the Earth, in terms of composition and surface pressure. Also, its seasonal cycle is similar, as Titan’ obliquity is about 27^°(23^°,5 for the Earth), although it is about 30 times as long. Titan’ haze exhibits an albedo contrast (NSA for North-South Asymmetry) that is changing seasonally. From the analysis of Voyager and Hubble Space Telescope data, we learned that at short visible wavelengths, the albedo of the winter hemisphere is lower by 10-20% than that of the summer hemisphere. This asymmetry peaks at 450 nm and reaches maximum amplitude around Titan’ equinoxes. It reverses in about five years, faster than a season which spans seven years. At longer wavelengths, longward of 700 nm, the asymmetry is inverted. The NSA reversal process in the red and in the UV seems to lead the reversal in the blue by 1 or 2 years. No valid explanation exists for this lag, at least in the red. The results from a recent model which couples atmospheric dynamics, haze microphysics and transport, as well as photochemistry, show that the NSA and its seasonal changes can be explained by an accumulation of haze particles at the winter pole. This is due to the pole-to-pole Hadley circulation pattern that is present during most of Titan’ year and rapidly disrupts at the time of the equinoxes. This model can also explain the observed cooler stratospheric temperatures and higher abundances of heavy hydrocarbons and nitriles in the winter polar region. In addition, it provides a mechanism for the formation of a detached haze layer around 300–400 km altitude, as well as the existence of a polar hood. Thus, it appears that the latitudinal contrasts we observe on Titan are conveniently tracing for us the dynamical behavior of its atmosphere.     

双向进气结构脉管制冷机直流形成机理

在脉管制冷机中,由双向进气结构诱发的直流流动,不仅会增加冷端换热器的负载,降低制冷机性能,而且还是引起制冷温度不稳定的重要原因。如何有效地抑制直流流动已成为脉管制冷机能否大规模应用的关键。而对直流形成机理进行全面、深入的研究是发展简单、有效直流抑制手段的前提。针对该研究热点,本文开展了双向进气结构脉管制冷机直流形成机理研究,基于流体网络理论,考察工质物性对直流的影响和作用机理,进一步揭示了直流的形成本质。     

基于流体网络理论的脉管制冷机调相机理

开展了脉管制冷机调相机理研究，从调相和调幅两方面出发，理论分析了各种形式脉管制冷机的调相特性，为探索其工作机理开辟了新途径。该方法很好地弥补了传统相位理论片面注重各种结构的调相功能而忽略其调幅功能的不足，更好地揭示了它们的作用机理．具有简单、直观的突出优点。进一步对其完善，该理论成果可用于脉管制冷机的定量设计和新结构的研发。     

JJ—7飞机对大气紊流的横航向响应及乘座品质计算

本文对JJ-7飞机的横航向晴空大气紊流响应及乘座品质进行了计算.计算结果表明,JJ-7飞机的横航向大气紊流响应值不大,乘座品质基本上满足要求,可以为飞行员接受.     

混合动力学中一种综合控制指标

本文从环境流体力学角度，结合混合动力学机理，导出了一种新混合综合控制指标。     

二维跨音速流动计算的显式多步有限面积方法

本文按Jameson等的思路,采用新的人工粘性项系数,建立显式多步有限面积方法,给出绕NACA0012翼型和RAE2822翼型跨音速流动的计算结果。     

基于模型降阶的随机最优输出反馈阵设计

本文研究了线性离散随机系统的模型降阶和最优输出反馈矩阵的设计问题。本文提出的设计方法不需要对原系统进行Anderson-Moore的迭代计算,直接利用求得的降阶模型解出近似的最优输出反馈阵。文中举例说明了设计方法的应用并进行了计算机仿真,仿真结果是令人满意的。