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Influence of small inertia on Jeffery orbits – CORRIGENDUM

Published online by Cambridge University Press:  11 November 2025

Davide Di Giusto*
Affiliation:
Aix Marseille Université, CNRS, IUSTI, Marseille, France Dipartimento Politecnico di Ingegneria e Architettura, University of Udine, Italy
Laurence Bergougnoux
Affiliation:
Aix Marseille Université, CNRS, IUSTI, Marseille, France
Cristian Marchioli
Affiliation:
Dipartimento Politecnico di Ingegneria e Architettura, University of Udine, Italy
Élisabeth Guazzelli
Affiliation:
Université Paris Cité, CNRS, Matière et Systèmes Complexes UMR 7057, Paris, France
*
Corresponding author: Davide Di Giusto, digiusto.davide@spes.uniud.it

Abstract

Information

Type
Corrigendum
Copyright
© The Author(s), 2025. Published by Cambridge University Press
Figure 0

Figure 1. Evolution of the components of the orientation vector ${\boldsymbol{n}}$, displayed as vertically aligned panels for 3 typical runs against the dimensionless time $t\dot \gamma $, for the fibre CYL10 with aspect ratio $r = 9$ and confinement ratio $\kappa = 0.19$: (a) $R{e_p} = 0.15$; (b) $R{e_p} = 1.0$. Comparison with the theory of Einarsson et al. (2015a), presented in ${\rm{\S}}$ B.1 is also given as black dashed lines. See Supplementary Materials for the directory of the figure including the data and the Jupyter notebook.

Figure 1

Figure 2. Evolution of the components of the orientation vector ${\boldsymbol{n}}$, displayed as vertically aligned panels for 3 typical runs against the dimensionless time $t\dot \gamma $, for the disk CYL005 with aspect ratio $r = 0.05$ and confinement ratio $\kappa = 0.19$: (a) $R{e_p} = 0.24$; (b) $R{e_p} = 0.8$. Comparison with the theory of Einarsson et al. (2015a), presented in ${\rm{\S}}$ ,B.1 is also given as black dashed lines. See Supplementary Materials for the directory of the figure including the data and the Jupyter notebook.

Figure 2

Figure 3. Evolution of the components of the orientation vector ${\boldsymbol{n}}$, displayed as vertically aligned panels for 3 typical runs against the dimensionless time $t\dot \gamma $, for the oblate spheroid ELL06 with aspect ratio $r = 0.6$ and confinement ratio $\kappa = 0.17$ at particle Reynolds number $R{e_p} = 0.43$. Comparison with the theory of Einarsson et al. (2015a), presented in ${\rm{\S}}$ ,B.1 is also given as black dashed lines. See Supplementary Materials for the directory of the figure including the data and the Jupyter notebook.

Figure 3

Figure 4. Experimental Jeffery orbits at two Reynolds numbers for the fibre CYL10 (top-row panels), the spheroid ELL06 (middle-row panels) and the disk CYL01 (bottom-row panels): (a) Fibre, $r = 9.0$, $R{e_p} = 0.08$; (b) Fibre, $r = 9.0$, $R{e_p} = 1.0$; (c) Spheroid, $r = 0.6$, $R{e_p} = 0.02$; (d) Spheroid, $r = 0.6$, $R{e_p} = 0.43$; (e) Disk, $r = 0.1$, $R{e_p} = 0.05$; (f) Disk, $r = 0.1$, $R{e_p} = 1.32$. The particles considered in this figure are shown in the vorticity-aligned position with their orientation vector ${\boldsymbol{n}}$ highlighted in cyan. The coloured dots represent the intersections of the axis given by the orientation vector ${\boldsymbol{n}}$ with the half sphere of radius $\ell $ for the prolate particles and $a$ for the oblate particles, respectively. The corresponding Jeffery orbits are also displayed as solid black lines and were obtained by integrating equation (1.1) from an initial condition given by the first flow-aligned orientation of each experiment. See Supplementary Materials for animations.

Supplementary material: File

Di Giusto et al. supplementary movie 1

Jeffery orbits for a fibre with equivalent aspect ratio r_eq=7.4 at small particle Reynolds number Re_p=0.08, run 5 of panel (a) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 2

Jeffery orbits for a fibre with equivalent aspect ratio r_eq=7.4 at small particle Reynolds number Re_p=0.08, run 6 of panel (a) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 3

Jeffery orbits for a fibre with equivalent aspect ratio r_eq=7.4 at small particle Reynolds number Re_p=0.08, run 8 of panel (a) of Figure 6;
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File 481.5 KB
Supplementary material: File

Di Giusto et al. supplementary movie 4

Jeffery orbits for a fibre with equivalent aspect ratio r_eq=7.4 at large particle Reynolds number Re_p=1.0, run 13 of panel (b) of Figure 6;
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Di Giusto et al. supplementary movie 5

Jeffery orbits for a fibre with equivalent aspect ratio r_eq=7.4 at large particle Reynolds number Re_p=1.0, run 14 of panel (b) of Figure 6;
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File 380.1 KB
Supplementary material: File

Di Giusto et al. supplementary movie 6

Jeffery orbits for a fibre with equivalent aspect ratio r_eq=7.4 at large particle Reynolds number Re_p=1.0, run 3 of panel (b) of Figure 6;
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File 472.3 KB
Supplementary material: File

Di Giusto et al. supplementary movie 7

Jeffery orbits for a spheroid with aspect ratio r=0.6 at small particle Reynolds number Re_p=0.02, run 1 of panel (c) of Figure 6;
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File 489 KB
Supplementary material: File

Di Giusto et al. supplementary movie 8

Jeffery orbits for a spheroid with aspect ratio r=0.6 at small particle Reynolds number Re_p=0.02, run 3 of panel (c) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 9

Jeffery orbits for a spheroid with aspect ratio r=0.6 at small particle Reynolds number Re_p=0.02, run 4 of panel (c) of Figure 6;
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File 875.8 KB
Supplementary material: File

Di Giusto et al. supplementary movie 10

Jeffery orbits for a spheroid with aspect ratio r=0.6 at moderate particle Reynolds number Re_p=0.43, run 10 of panel (d) of Figure 6;
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File 1.1 MB
Supplementary material: File

Di Giusto et al. supplementary movie 11

Jeffery orbits for a spheroid with aspect ratio r=0.6 at moderate particle Reynolds number Re_p=0.43, run 8 of panel (d) of Figure 6;
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File 1.2 MB
Supplementary material: File

Di Giusto et al. supplementary movie 12

Jeffery orbits for a spheroid with aspect ratio r=0.6 at moderate particle Reynolds number Re_p=0.43, run 5 of panel (d) of Figure 6
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File 652.1 KB
Supplementary material: File

Di Giusto et al. supplementary movie 13

Jeffery orbits for a disk with equivalent aspect ratio r=0.18 at small particle Reynolds number Re_p=0.05, run 1 of panel (e) of Figure 6;
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Di Giusto et al. supplementary movie 14

effery orbits for a disk with equivalent aspect ratio r=0.18 at small particle Reynolds number Re_p=0.05, run 2 of panel (e) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 15

Jeffery orbits for a disk with equivalent aspect ratio r=0.18 at small particle Reynolds number Re_p=0.05, run 5 of panel (e) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 16

Jeffery orbits for a disk with equivalent aspect ratio r=0.18 at large particle Reynolds number Re_p=1.32, run 1 of panel (e) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 17

Jeffery orbits for a disk with equivalent aspect ratio r=0.18 at large particle Reynolds number Re_p=1.32, run 2 of panel (e) of Figure 6;
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Supplementary material: File

Di Giusto et al. supplementary movie 18

Jeffery orbits for a disk with equivalent aspect ratio r=0.18 at large particle Reynolds number Re_p=1.32, run 9 of panel (e) of Figure 6;
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Di Giusto et al. supplementary material

Di Giusto et al. supplementary material
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Di Giusto et al. supplementary material

Di Giusto et al. supplementary material

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