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Flow-induced motions of flexible plates: fluttering, twisting and orbital modes

Published online by Cambridge University Press:  07 February 2019

Yaqing Jin
Affiliation:
Mechanical Science and Engineering Department, University of Illinois, Urbana, IL 61801, USA
Jin-Tae Kim
Affiliation:
Mechanical Science and Engineering Department, University of Illinois, Urbana, IL 61801, USA
Shifeng Fu
Affiliation:
Mechanical Science and Engineering Department, University of Illinois, Urbana, IL 61801, USA College of Water Conservancy and Hydropower Engineering, Hohai University, Nanjing 210024, China
Leonardo P. Chamorro*
Affiliation:
Mechanical Science and Engineering Department, University of Illinois, Urbana, IL 61801, USA Civil and Environmental Engineering Department, University of Illinois, Urbana, IL 61801, USA Aerospace Engineering Department, University of Illinois, Urbana, IL 61801, USA
*
†Email address for correspondence: lpchamo@illinois.edu

Abstract

The unsteady dynamics of wall-mounted flexible plates under inclined flows was fundamentally described using theoretical arguments and experiments under various Cauchy numbers $Ca=\unicode[STIX]{x1D70C}_{f}bL^{3}U_{0}^{2}/(EI)\in [7,81]$ (where $\unicode[STIX]{x1D70C}_{f}$ is the fluid density, $b$ and $L$ are the plate width and length, $U_{0}$ is the incoming velocity, $E$ is Young’s modulus and $I$ is the second moment of the area) and inclination angles $\unicode[STIX]{x1D6FC}$. Three-dimensional particle tracking velocimetry and a high-resolution force sensor were used to characterize the evolution of the plate dynamics and aerodynamic force. We show the existence of three distinctive, dominant modes of tip oscillations, which are modulated by the structure dynamic and flow instability. The first mode is characterized by small-amplitude, planar fluttering-like motions occurring under a critical Cauchy number, $Ca=Ca_{c}$. Past this condition, the motions are dominated by the second mode consisting of unsteady twisting superimposed onto the fluttering patterns. The onset of this mode is characterized by a sharp increase of the force fluctuation intensity. At sufficiently high $Ca$ and $\unicode[STIX]{x1D6FC}$, the plate may undergo a third mode given by large-scale tip orbits about the mean bending. Using the equation of motion and first-order approximations, we propose a formulation to estimate $Ca_{c}$ as a function of $\unicode[STIX]{x1D6FC}$; it exhibits solid agreement with experiments.

Information

Type
JFM Papers
Copyright
© 2019 Cambridge University Press 
Figure 0

Figure 1. (a) Schematic of the experimental set-up illustrating the force sensor, rotary table and PTV system. (b) Basic definitions; the origin of the coordinate system is fixed at the centre of the plate base, the black and red fiducial points denote the tips used in other figures, and $\unicode[STIX]{x1D6FC}$ is the inclination angle at the plate base with respect to the mean flow $U_{0}$.

Figure 1

Figure 2. (a) The normal-force coefficient ($C_{N}$) for various $Ca$ and $\unicode[STIX]{x1D6FC}$. (b) Intensity of the normal-force fluctuations ($I_{N}$) across various $Ca$ and $\unicode[STIX]{x1D6FC}$. (c,d) Sample time series of the normal force $F_{N}$ at the plate base right below ($Ca=20.5$ for panel c) and above ($Ca=24$ for panel d) $Ca_{c}$ at $\unicode[STIX]{x1D6FC}=45^{\circ }$. (e–g) Snapshots of plate dynamics at $\unicode[STIX]{x1D6FC}=45^{\circ }$ and various $Ca$: (e) $Ca=9$, (f) $Ca=32$ and (g) $Ca=68$. Here (i), (ii) and (iii) are instants highlighting dominant modes of tip motion.

Figure 2

Figure 3. Trajectories of the tips for various $\unicode[STIX]{x1D6FC}$ and $Ca$: (a–c) $\unicode[STIX]{x1D6FC}=0^{\circ }$ with $Ca=7$, 41 and 68; (d–f) same as (a–c) with $\unicode[STIX]{x1D6FC}=30^{\circ }$; (g–i) same as (a–c) with $\unicode[STIX]{x1D6FC}=45^{\circ }$. Here $x^{\ast }=x/L$, $y^{\ast }=y/L$ and $z^{\ast }=z/L$ denote the normalized tip locations. The blue lines represent the location of the plate base.

Figure 3

Figure 4. Sampled tip trajectories and normalized streamwise velocity spectra $\unicode[STIX]{x1D6F7}^{\ast }=\unicode[STIX]{x1D6F7}/\text{max}\{\unicode[STIX]{x1D6F7}\}$ of a tip under (a) $Ca=7$ and $\unicode[STIX]{x1D6FC}=0^{\circ }$, (b) $Ca=41$ and $\unicode[STIX]{x1D6FC}=30^{\circ }$, (c) $Ca=41$ and $\unicode[STIX]{x1D6FC}=45^{\circ }$, and (d) $Ca=68$ and $\unicode[STIX]{x1D6FC}=45^{\circ }$. The colour bar indicates the normalized height difference between the tips ($\unicode[STIX]{x0394}z_{t}^{\ast }$). The two-headed blue arrow in (b) denotes the twisting oscillations, whereas the anticlockwise arrow in (d) indicates the 3D orbital motion of the tips composed of three stages. The insets show the (red) tip streamwise velocity $u_{t}$.

Figure 4

Figure 5. Normalized base normal-force spectra $\unicode[STIX]{x1D6F7}_{N}^{\ast }=\unicode[STIX]{x1D6F7}/\text{max}\{\unicode[STIX]{x1D6F7}\}$ at $\unicode[STIX]{x1D6FC}=45^{\circ }$ and (a) $Ca=36.3$, (b) $Ca=38.6$ and (c) $Ca=41$. The dashed arrows indicate the gradual increase of the frequency component corresponding to the orbital motions.

Figure 5

Figure 6. Instantaneous tip heights $z^{\ast }=z/L$ during one representative orbital cycle under $Ca=68$ and $\unicode[STIX]{x1D6FC}=45^{\circ }$; here $T_{r}=1/f_{r}$ is the period of orbital motion. The black and red points denote each tip.

Figure 6

Figure 7. (a) Schematic illustrating parameters near plate tip region with bending angle $\unicode[STIX]{x1D703}$. (b) Schematic of the cross-section of the plate undergoing twisting motion under the influence of instantaneous angular velocity. The ‘$+$’ symbol denotes the plate centre. (c) Distribution of the plate tips projected in the $x{-}z$ plane under $Ca=7$ and (i) $\unicode[STIX]{x1D6FC}=0^{\circ }$, (ii) $\unicode[STIX]{x1D6FC}=30^{\circ }$ and (iii) $\unicode[STIX]{x1D6FC}=45^{\circ }$. (d) Distribution of $C_{M}=2M/(\unicode[STIX]{x1D70C}_{f}U_{0}^{2}b^{2}L)$ with $\unicode[STIX]{x1D6FC}$ of a rigid plate with the same geometry.

Figure 7

Figure 8. $Ca_{c}$ and dimensionless quantity $C_{t}$ (3.9) characterizing the threshold of twisting motions; the dashed line marks the averaged value of $C_{t}$ across $\unicode[STIX]{x1D6FC}$.

Jin et al. supplementary movie 1

Raw video illustrating small-amplitude fluttering. This sample movie is played 8x slower.

Download Jin et al. supplementary movie 1(Video)
Video 2.9 MB

Jin et al. supplementary movie 2

Raw video illustrating twisting oscillations. This sample movie is played 8x slower.

Download Jin et al. supplementary movie 2(Video)
Video 2.9 MB

Jin et al. supplementary movie 3

Raw video illustrating large-scale orbital motions. This sample movie is played 8x slower.

Download Jin et al. supplementary movie 3(Video)
Video 2.9 MB