Flutter analysis of an airfoil with bounded random parameters in incompressible flow via Gegenbauer polynomial approximation

The effects of parameter uncertainty on the flutter characteristics of a two-dimensional airfoil in an incompressible flow were investigated through Gegenbauer polynomial approximation. The uncertain parameters, such as the linear and cubic pitch stiffness coefficients are modeled as bounded random variables with λ-PDFs (probability density functions). With the aid of Gegenbauer polynomial approximation, the two-dimensional stochastic airfoil system is transformed at first into its equivalent deterministic one. Then the Hopf-bifurcation point is determined through the equivalent deterministic system, and the onset of the flutter, together with the flutter frequency against the probability density distribution parameter and the intensity of the random variable is explored. In addition, the ranges of the peak pitch and plunge responses against the flight speed and the PDFs of the peak pitch response are obtained. Numerical results show how the probability density distribution parameters and the intensities of random parameters affect the flutter onset speed, flutter angular frequency, the upper and lower boundaries of peak responses, and the PDFs of peak responses.     

基于TMS320C80的BP算法并行实现的研究

结合 TMS32 0 C80的编程结构 ,利用神经网络的权并行性和神经元并行性 ,提出了BP算法的并行实现方法 ,并解决了存储器访问冲突、数据双缓冲传输、PP细粒度并行和死锁等问题。结果表明 ,该并行 BP算法十分有效。     

自适应直角切割网格民机增升装置绕流数值模拟

提出并介绍了基于直角切割网格的分区面搭接技术,采用变长宽比网格方法,成功地进行了存在外形间断(剪刀叉)的民机增升装置的网格生成和绕流Euler方程数值模拟.根据外形的特点,运用"根"网格分区算法,降低了整个网格的生成难度;通过基于外形的自适应网格加密技术,详细地描述了外形上的大量缝道和凹槽,提高了网格质量;在分区交界面上,利用重叠面积切割和面搭接算法实现了两侧网格间的流场信息传递,并保证了通量守恒;采用中心有限体积方法,结合双时间推进算法,完成流场的Euler方程数值模拟,计算结果与实验数据吻合良好,说明所述方法的正确性.     

三维可压缩混合层中扰动演化的研究

为了利用被动控制增强可压缩混合层中混合效率,本文用数值模拟的方法研究了三维可压缩混合层中扰动向下游的演化.通过在入口处引入不同的不稳定T-S波,给出了扰动随空间的演化过程,及马赫数对扰动演化的影响.计算结果表明在马赫数较小时,扰动波增长很快,当马赫数增大时,扰动所形成的流向涡的强度会减弱.这一结论与流动稳定性分析结果是一致的.     

连续自由流电泳微重力下分离模式蛋白质的研究

以连续自由流电泳的区带电泳模式分离血红蛋白和细胞色素C，比较了不同缓冲液甘油浓度下的分离效果，确定了最终装载在神舟4号飞船上A3—2型电泳仪的电泳分离条件，通过地面和空间实验，初步探讨了微重力对连续自由流电泳分离的影响，并对电泳的分离产物做了多种检测．     

一种航天测控冗余跟踪弧段处理方法

随着在轨航天器的日益增多,测控资源的需求量也日益增大,因此,其使用效率也倍受关注。当航天器重要测控弧段安排多个测控设备进行全力跟踪时,很容易出现测控弧段搭接或完全被覆盖的情况。为有效利用现有测控资源,针对弧段搭接的情况,提出了一种基于冗余度评价函数的跟踪弧段处理方法,该方法在不降低跟踪总时长情况下,通过合理有效地配置测控资源,剔除了冗余跟踪弧段,提高了现有测控资源的使用效率。     

基于3D打印技术的微波开关设计与实践

文章介绍了一种基于3D打印技术的R型波导开关的设计方法,并对影响微波开关性能指标的射频参数、切换时间进行了验证。验证结果表明,微波开关的射频指标无恶化,切换时间缩短,微波开关可靠性得到提升。通过3D打印技术的应用,减轻开关重量17%以上,生产周期缩短60%以上。文章论述了微波开关射频指标、切换时间的设计过程和验证结果,解决了X频段R型波导开关切换时间长和重量大的不足,为波导微波开关制造提供了一种新的途径。     

Fe3Si基合金降低温轧温度的研究

研究了不同轧制工艺和热处理工艺对Fe3Si基合金塑性的影响,室温拉伸和高温拉伸实验结果表明,水冷的热处理工艺使Fe3Si基合金的塑性得到很大的提高,使可轧制的温度降低到300℃。     

图像序列中机动目标三维运动和结构的计算

综合视觉运动分析中的2类处理方法,选取图像中的角点作为特征点,在理论上证明了图像序列的光流场可以近似地用角点的位移场代替。利用已有文献中的建模思想,详细推导出递归计算机动目标三维运动和结构的非线性计算模型,采用广义卡尔曼滤波(EKF)递归地计算图像序列中机动目标的三维运动和结构。合成图像序列和真实图像序列实验结果表明该算法能取得较好的效果。     

Analytic and numerical treatment of motion of dust grain particle around triangular equilibrium points with post-AGB binary star and disc

This paper investigates the motion around the triangular equilibrium points, of a passively gravitating dust particle in the gravitational field of a low-mass post-AGB binary system, surrounded by circumbinary disc. The two bodies of the binary are modeled as a triaxial star and a radiating-oblate star. Due to small deviation of disc stars on circular orbits, we have assumed that the Coriolis and centrifugal forces of the stars are slightly perturbed. The triangular equilibrium points of the particle are found. These points are defined by, triaxiality of the primary star, oblateness and radiation of the secondary one and the gravitational potential from the disc mass. Further, when the disc mass increases, the particle moves nearer to the stars and farther away from the disc. In general, these equilibrium points are linearly stable when μ < μ_C; where μ is the mass ratio and μ_C is the critical mass function, defined by the parameters of the system. The effects of each of these parameters on the size of the stability region are stated, and the periodic motion around the stable points is examined. It is seen that the orbits are ellipses, and the orientation, eccentricities, lengths of the semi-major and semi-minor axes are influenced by the parameters of the problem. In particular, for our numerical linear stability analysis, we have taken an extremely depleted pulsating star, IRAS 11472-0800 as the post-AGB triaxial star, with a weakly-radiating young white dwarf star; G29-38 as the secondary. For this system, the stability result of the triangular points comes out different. Here, μ_C < μ throughout the entire range of the mass ratio and the critical mass function. Hence, the triangular equilibrium points are unstable. The stability of the orbits is tested using the Poincaré surfaces of section (Pss). The region of stability is controlled by the introduced parameters and the Jacobi constant.