Flow around an inclined circular disk

Song Gao, Longbin Tao, Xinliang Tian, Jianmin Yang

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Abstract

Direct numerical simulations are performed for the uniform flow around an inclined circular disk. The diameter–thickness aspect ratio ( X=D/td) of the disk is 50 and the inclination angle (\alpha) is considered over the range of 0<6<80 deg, where \alpha=0 deg refers to the condition where the flow is normal to the disk. The Reynolds number (Re), based on the short axis of projection in the streamwise direction, is defined as Re=U_\inf D cos \alpha /\mu, where U_\inf is the velocity of the flow and \mu is the kinematic viscosity. Re is investigated over the range of 50 < Re < 300. In the considered Re–\alpha parametric space, five states are observed and denoted as: (I) steady state (SS); (II) periodic state (PS); (III) periodic state with a low frequency modulation (PSL); (IV) quasi-periodic state (QP) and (V) chaotic state (CS). Both Re and \alpha affect the bifurcation mechanism. The bifurcating sequence occurring at \alpha=0 deg is generally observed over the whole Re–\alpha space, although it is advanced at small \alpha and delayed at large \alpha. The advancement of thresholds for different states is due to the effects introduced by inclination, which tend to select the plane of symmetry for the wake in order to regulate the wake and intensify some flow features. Nevertheless, the bifurcations are still in the dominant position when leading a state without stable symmetry, i.e. the planar symmetry could not be recovered by small \alpha. These phenomena are further discussed with respect to the vortex shedding patterns behind the disk. Furthermore, for any fixed disk, the wake behaviour is only associated with that found in the steady vertical state of a freely falling disk. The fully coupled fluid–body system is fundamentally different from the fixed cases.
Original languageEnglish
Pages (from-to)687-714
Number of pages28
JournalJournal of Fluid Mechanics
Volume851
Early online date31 Jul 2018
DOIs
Publication statusPublished - 25 Sep 2018

Fingerprint

wakes
Vortex shedding
Direct numerical simulation
Frequency modulation
inclination
Aspect ratio
Reynolds number
symmetry
Viscosity
uniform flow
vortex shedding
direct numerical simulation
falling
frequency modulation
aspect ratio
kinematics
projection
viscosity
low frequencies
thresholds

Keywords

  • bifurcation
  • vortex instability
  • wakes

Cite this

Gao, Song ; Tao, Longbin ; Tian, Xinliang ; Yang, Jianmin. / Flow around an inclined circular disk. In: Journal of Fluid Mechanics. 2018 ; Vol. 851. pp. 687-714.
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Flow around an inclined circular disk. / Gao, Song; Tao, Longbin; Tian, Xinliang; Yang, Jianmin.

In: Journal of Fluid Mechanics, Vol. 851, 25.09.2018, p. 687-714.

Research output: Contribution to journalArticle

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T1 - Flow around an inclined circular disk

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AU - Tao, Longbin

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AU - Yang, Jianmin

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AB - Direct numerical simulations are performed for the uniform flow around an inclined circular disk. The diameter–thickness aspect ratio ( X=D/td) of the disk is 50 and the inclination angle (\alpha) is considered over the range of 0<6<80 deg, where \alpha=0 deg refers to the condition where the flow is normal to the disk. The Reynolds number (Re), based on the short axis of projection in the streamwise direction, is defined as Re=U_\inf D cos \alpha /\mu, where U_\inf is the velocity of the flow and \mu is the kinematic viscosity. Re is investigated over the range of 50 < Re < 300. In the considered Re–\alpha parametric space, five states are observed and denoted as: (I) steady state (SS); (II) periodic state (PS); (III) periodic state with a low frequency modulation (PSL); (IV) quasi-periodic state (QP) and (V) chaotic state (CS). Both Re and \alpha affect the bifurcation mechanism. The bifurcating sequence occurring at \alpha=0 deg is generally observed over the whole Re–\alpha space, although it is advanced at small \alpha and delayed at large \alpha. The advancement of thresholds for different states is due to the effects introduced by inclination, which tend to select the plane of symmetry for the wake in order to regulate the wake and intensify some flow features. Nevertheless, the bifurcations are still in the dominant position when leading a state without stable symmetry, i.e. the planar symmetry could not be recovered by small \alpha. These phenomena are further discussed with respect to the vortex shedding patterns behind the disk. Furthermore, for any fixed disk, the wake behaviour is only associated with that found in the steady vertical state of a freely falling disk. The fully coupled fluid–body system is fundamentally different from the fixed cases.

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