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首页> 外文期刊>International Journal of Heat and Fluid Flow >Laminar flow structures from a rotating sphere: Effect of rotating axis angle
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Laminar flow structures from a rotating sphere: Effect of rotating axis angle

机译:旋转球面的层流结构:旋转轴角的影响

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摘要

A Fourier-Chebyshev spectral collocation method is used to compute the flow past a steadily rotating sphere subjected to a uniform cross flow. The simulations are performed at Reynolds numbers Re = 100,250 and 300, where the Reynolds number is based on freestream velocity and sphere diameter. These Reynolds numbers cover three different flow regimes for a stationary sphere, from steady axisym-metric, steady planar-symmetric to unsteady planar-symmetric. The effect of varying the rotation axis angle, α, on the laminar flow structures and time-averaged hydrodynamic forces is investigated over a range of non-dimensional rotation rates, Ω.~* This study reveals the time-averaged flight path of a solid rotating particle.rnAt Re = 100, the flow is always steady. The near-wake projected streamline patterns and pressure coefficient contours are topologically similar at α = 0 independent of the range of Ω~* considered. As α increases, the near-wake recirculation bubble is either suppressed or shifted and thus affects the pressure recovery behind the sphere. This in turn affects both the drag and lift coefficients, C_D and C_L. For all Ω~* considered, C_D and C_L increase as α increases and the increment is more pronounced at higher Ω~* At Re = 250 and 300, calculations show both steady and unsteady wake structures. The state of the wake structures depends strongly on α and Ω~*. However, the time-averaged flow fields are qualitatively similar to Re = 100. As a result, the time averaged drag and lift coefficients, C_D and C_L follow the same trend as at Re = 100. The increase in Re dramatically reduce the C_D compared to the same Ω~* and α at Re = 100. C_L shows a more complicated behaviour as Re increases.
机译:傅里叶-切比雪夫光谱搭配方法用于计算经过稳定旋转球体的,经过均匀横流的流量。在雷诺数Re = 100,250和300时执行模拟,其中雷诺数基于自由流速度和球体直径。这些雷诺数涵盖了固定球体的三种不同流动形式,从稳定的轴对称,稳定的平面对称到不稳定的平面对称。研究了在一系列无量纲旋转速率Ω的情况下,改变旋转轴角α对层流结构和时间平均流体动力的影响。〜*该研究揭示了固体的时间平均飞行路径在Re = 100时,流量始终稳定。与α〜*的范围无关,在α= 0时,近苏醒的投影流线样式和压力系数轮廓在拓扑上相似。随着α的增加,接近尾迹的再循环气泡被抑制或移动,从而影响球体后的压力恢复。这继而影响阻力系数和提升系数C_D和C_L。对于所有考虑的Ω〜*,C_D和C_L随α的增加而增加,并且在Ω〜*较高的情况下增加更为明显。在Re = 250和300时,计算结果显示了稳定和非稳定的尾流结构。尾波结构的状态在很大程度上取决于α和Ω〜*。但是,时间平均流场在质量上类似于Re =100。因此,时间平均阻力和升力系数C_D和C_L遵循与Re = 100相同的趋势。与之相比,Re的增加大大降低了C_D当Re = 100时,C_L表现出更复杂的行为。

著录项

  • 来源
    《International Journal of Heat and Fluid Flow 》 |2010年第5期| p.961-972| 共12页
  • 作者单位

    Department of Mechanical Engineering, University of Melbourne, Parkville, VIC 3010, Australia;

    rnDepartment of Mechanical Engineering, University of Melbourne, Parkville, VIC 3010, Australia;

    rnAir Vehicles Division, Defence Science & Technology Organisation, 506 Lorimer St., Fishermans Bend, VIC 3207, Australia;

    rnCSIRO Mathematics, Informatics & Statistics, Clayton, VIC 3168, Australia;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    laminar flow; sphere; rotating axis angle;

    机译:层流球;旋转轴角度;

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