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Numerical Investigations of Transition in Hypersonic Flows over Circular Cones

机译:圆锥上超音速流过渡的数值研究

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摘要

This thesis focuses on secondary instability mechanisms of high-speed boundary layers over cones with a circular cross section. Hypersonic transition investigations at Mach 8 are performed using Direct Numerical Simulations (DNS). At wind-tunnel conditions, these simulations allow for comparison with experimental measurements to verify fundamental stability characteristics.To better understand geometrical influences, flat-plate and cylindrical geometries are studied using after-shock conditions of the conical investigations. This allows for a direct comparison with the results of the sharp cone to evaluate the influence of the spanwise curvature and the cone opening angle. The ratio of the boundary-layer thickness to the spanwise radius is used to determine the importance of spanwise curvature effects. When advancing in the downstream direction the radius increaseslinearly while the boundary-layer thickness stays almost constant. Hence, spanwise curvature effects are strongest close to the nose and decrease in downstream direction. Their influences on the secondary instability mechanisms provide some rudimentary guidance in the design of future high-speed air vehicles.In experiments, blunting of the nose tip of the circular cone results in an increase in critical Reynolds number (c.f. Stetson et al. (1984)). However, once a certain threshold of the nose radius is exceeded, the critical Reynolds number decreases even to lower values than for the sharp cone. So far, conclusive explanations for this behavior could not be derived based on the available experimental data. Therefore, here DNS is used to study the effect of nose bluntness on secondary instability mechanisms in order to shed light on the underlying flow physics. To this end, three different nose tip radii are considered-the sharp cone, a small nose radius and a large nose radius. A small nose radius moves the transition on-set downstream, while for a large nose radius the so-called transition reversal is observed. Experimentalists hold influences of the entropy layer responsible but detailed numerical studies may lead to alternateconclusions.
机译:本文主要研究具有圆形横截面的圆锥体上高速边界层的次要失稳机理。使用直接数值模拟(DNS)进行8马赫的高超音速过渡研究。在风洞条件下,这些模拟可以与实验测量结果进行比较,以验证基本的稳定性特征。为了更好地理解几何影响,使用圆锥调查的余震条件研究了平板和圆柱几何形状。这样可以直接与尖锥的结果进行比较,以评估翼展方向曲率和锥张角的影响。边界层厚度与翼展方向半径的比率用于确定翼展方向曲率效应的重要性。当沿下游方向前进时,半径线性增加,而边界层厚度几乎保持恒定。因此,翼展方向曲率效应在靠近鼻子处最强,并在下游方向减小。它们对次级失稳机制的影响为未来的高速飞行器设计提供了基本的指导。在实验中,圆锥形鼻尖的钝化导致临界雷诺数增加(参见Stetson等人(1984) ))。但是,一旦超过某个特定的鼻半径阈值,临界雷诺数就会降低,甚至降低到比尖锥更低的值。到目前为止,无法根据可用的实验数据得出对此行为的结论性解释。因此,此处使用DNS研究鼻子钝性对继发性不稳定性机制的影响,以阐明潜在的流动物理学。为此,考虑了三个不同的鼻尖半径-尖锥,较小的鼻腔半径和较大的鼻腔半径。较小的机头半径将过渡过渡到下游,而对于较大的机头半径,则观察到所谓的过渡反转。实验学家认为熵层的影响是负责任的,但是详细的数值研究可能会导致其他结论。

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    Husmeier Frank;

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  • 年度 2008
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