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71.
局部附面层吸除对高负荷扩压叶栅气动性能的影响 总被引:1,自引:0,他引:1
实验研究了低速条件下局部附面层吸除对高负荷扩压叶栅气动性能的影响.采用五孔气动探针测量了叶栅出口截面气动参数,并对叶片表面静压进行了测量,详细分析了局部吸气方式、吸气量和吸气位置对叶栅出口截面总压损失和负荷能力的影响.结果表明,采用吸力面两端吸气和中间吸气方式均能够有效吸除叶栅流道内低能流体,增加叶栅的气动负荷,从而提高叶栅的气动性能;采用吸力面两端吸气对叶栅气动性能的改善要优于吸力面中间吸气;叶栅气动性能的改善主要在靠近叶展中部区域,而对角区核心区和端部区域的影响并不明显. 相似文献
72.
The purpose of this work is to improve the k-ω-γ transition model for separationinduced transition prediction. The fundamental cause of the excessively small separation bubble predicted by k-ω-γ model is scrutinized from the perspective of model construction. On the basis,three rectifications are conducted to improve the k-ω-γ model for separation-induced transition.Firstly, a damping function is established via comparing the molecular diffusion timescale with the rapid pressure-strain timescale... 相似文献
73.
During the flight of the aircraft, the pilot must repeat the instruction sent by the controller, and the controller must further confirm these read-backs, in this way to further ensure the safety of air transportation. However, fatigue, tension, negligence and other human factors may prevent the controller from realizing read-back errors in time, which is a huge hidden danger for the safety of civil aviation transportation. This paper proposes a novel strategy to implement fine-grained semantic ... 相似文献
74.
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76.
运用爆破震动来识别地下裂隙和软弱夹层 总被引:1,自引:0,他引:1
从爆破震动信号主要来源于爆破区邻近范围内地质结构的自振的观点出发,提出了一种探测地下裂隙和软弱夹层的新技术:把震源布置在裂隙和软弱夹层附近进行爆破,由于介质中裂隙和软弱夹层的存在使得局部结构的刚度减小,直接影响到爆破介质振动的速度幅值和频率,因此可以通过地表接收器接收的振动信号(包括振动速度的幅值和频率)识别出裂隙和软弱夹层的大小和形状等特征.通过无网格的数值算例分别从水平裂隙和斜裂隙的情况下总结规律说明了这种方法的可行性. 相似文献
77.
后向台阶层流边界层分离实验研究 总被引:5,自引:1,他引:5
本文应用偏振差动式激光测速仪对后向台阶层流边界层分离、再附及发展为湍流边界层的整个过程进行了精细的量测,得到了时均速度、湍流强度等的分布特性。我们发现,在本实验条件下,层流边界层分离后在再附点处为过渡流,进一步发展最后形成湍流边界层。在湍流边界层区域,流速分布遵循对数律,但积分常数比平板湍流边界层中所得值要大。 相似文献
78.
Numerical simulations were carried out to investigate the effects of synthetic jet actuation frequency on the separated flow in a diffusing S-duct. The Reynolds number based on the entrance height was 9.78×105. At first, the numerical model was validated with experimental data, and then, the interaction between the separated flow and the synthetic jets at different frequencies was discussed. The results demonstrate that the control effect is significantly dependent on the momentum mixing enhancement between inside of the separated boundary layer and the outer flow. There exists a narrow range of actuation frequency, in which effective separation control can be achieved using synthetic jets. A dimensionless frequency F+=1.0 is identified as the optimal frequency, with a momentum coefficient of 1.62×10-3, the separation area is reduced about 46%, and the aerodynamic performance of the S-duct is also greatly improved compared to uncontrolled case. Further analysis reveals that the choice of actuation frequency is mainly determined by the momentum flux produced by a single ejection and the spacing between adjacent ejections, the optimal frequency case can be understood as a balance between the two factors. In addition, it is found that the synthetic jets can also suppress the secondary flows while decreasing the separation. 相似文献
79.
应用Strawn&.Kline的准同时粘性/无粘流匹配模型,于动量积分布方程中加入了曲率和雷诺正应力两个二阶修正项,计算了二维不可压湍流附面层分离流地。文中首先分析推导了新的曲率修正公式,给出了两个算例,比较了修正项对计算结果的影响,并与实验做了对比。 相似文献
80.
The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field. 相似文献