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TIP VORTEX CAVITATION INCEPTION SCALING FOR HIGH REYNOLDS NUMBER APPLICATION

机译:尖端涡旋空化初始化高雷诺数应用程序的缩放

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Tip vortices that are generated by marine lifting surfaces such as propeller blades, ship rudders, hydrofoil wings, and anti-roll fins can lead to cavitation. Prediction of the onset of this cavitation depends on model tests at Reynolds numbers much lower than those for the corresponding full-scale flows. The effect of Reynolds number variations on the scaling of tip vortex cavitation inception is investigated using a theoretical flow similarity approach. The ratio of the circulations in the full-scale and model-scale trailing vortices is obtained by assuming that the spanwise section lift coefficient distributions are the same between model and full-scale. The vortex pressure distributions and core sizes are derived using the Rankine vortex model and McCormick's assumption about the dependence of the vortex core size 9n the boundary layer thickness at the tip region. Using a logarithmic law to describe the velocity profile in the boundary layer over a large range of Reynolds number, the boundary layer thickness becomes dependent on the Reynolds number to a varying power. In deriving the cavitation inception scaling in the traditional scaling format of σ_(if) / σ_(im)= (Re_f/Re_m)~n, the values of n are not constant and depend on the values of Ref and Rem themselves. This contrasts traditional scaling for which n is treated as a fixed value that is independent of Reynolds numbers. At very high Reynolds numbers, the present theory predicts the value of n to approach zero, consistent with the trend of these flows to become inviscid. Comparison of the present theory with available experimental data shows promising results, especially with recent results from high Reynolds number tests. Numerical examples are given of the values of n for different model to full-scale sizes and Reynolds numbers.
机译:由乘船叶片,船舵,水翼翼和防侧翅片产生的海洋提升表面产生的尖端涡流可以导致空化。预测该空化的开始取决于雷诺数的模型测试远低于相应的全尺度流的雷诺数。利用理论流动相似性方法研究了雷诺数数变化对尖端涡旋空化初始化的缩放的影响。通过假设模型和满量程之间的翼展部分提升系数分布相同,获得了全尺度和模型落后涡流中的循环中的循环比率。涡流压力分布和核心尺寸是使用Rankine Vortex Model和McCormick关于涡旋芯尺寸9N在尖端区域的边界层厚度的依赖性的假设来得出的。使用对数定律在大范围的雷诺数中描述边界层中的速度分布,边界层厚度变得取决于雷诺数到不同的功率。在Σ_(if)/σ_(im)=(re_f / re_m)〜n的传统缩放格式中导出空化初始化缩放,n的值不是恒定的并且取决于REF和REM的值。这对比传统的缩放被视为与雷诺数无关的固定值。在非常高的雷诺数,本文预测n接近零的值,与这些流动的趋势变得无粘性。本理论与可用实验数据的比较显示了有希望的结果,特别是近期雷诺数测试的结果。向全尺寸尺寸和雷诺数的不同模型的N值给出数值例。

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