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On the lift-optimal aspect ratio of a revolving wing at low Reynolds number

Jardin, Thierry and Colonius, Tim On the lift-optimal aspect ratio of a revolving wing at low Reynolds number. (2018) Journal of the Royal Society Interface, 15 (143). 1-31. ISSN 1742-5689

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Official URL: https://doi.org/10.1098/rsif.2017.0933

Abstract

Lentink & Dickinson (2009) showed that rotational acceleration stabilized the leading-edge vortex on revolving, low-aspect-ratio wings, and hypothesized that a Rossby number of around three, which is achieved during each half-stroke for a variety of hovering insects, seeds, and birds, represents a convergent high-lift solution across a range of scales in nature. Subsequent work has verified that, in particular, the Coriolis acceleration plays a key role in LEV stabilization. Implicit in these results is that there exists an optimal aspect ratio for wings revolving about their root, because it is otherwise unclear why, apart from possible morphological reasons, the convergent solution would not occur for an even lower Rossby number. We perform direct numerical simulations of the flow past revolving wings where we vary the aspect ratio and Rossby numbers independently by displacing the wing root from the axis of rotation. We show that the optimal lift coefficient represents a compromise between competing trends with competing time scales where the coefficient of lift increases monotonically with aspect ratio, holding Rossby number constant, but decreases monotonically with Rossby number, when holding aspect ratio constant. For wings revolving about their root, this favors wings of aspect ratio between three and four.

Item Type:Article
Audience (journal):International peer-reviewed journal
Uncontrolled Keywords:
Institution:Université de Toulouse > Institut Supérieur de l'Aéronautique et de l'Espace - ISAE-SUPAERO (FRANCE)
Other partners > California Institute of Technology - Caltech (USA)
Laboratory name:
Funders:
Fondation ISAE-Supaero
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Deposited By: Thierry Jardin
Deposited On:07 Dec 2018 08:57

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