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The inter-scale energy budget in a von Kármán mixing flow

The inter-scale energy budget in a von Kármán mixing flow
The inter-scale energy budget in a von Kármán mixing flow

A detailed assessment of the inter-scale energy budget of the turbulent flow in a von Kármán mixing tank has been performed based on two extensive experimental data sets. Measurements were performed at a Taylor microscale Reynolds number of in the central region of the tank, using scanning particle image velocimetry (PIV) to fully resolve the velocity gradient tensor (VGT), and stereoscopic PIV for an expanded field of view. Following a basic flow characterisation, the Kármán-Howarth-Monin-Hill equation was used to investigate the inter-scale energy transfer. Access to the full VGT enabled the contribution of the different terms of the energy budget to be evaluated without any assumptions or approximations. The scale-space distribution of the dominant terms was also reported to assess the isotropy of the energy transfer. The results show a highly anisotropic distribution of energy transfer in scale space. Energy transfer was shown in a spherically averaged sense to be dominated at the small scales by the nonlinear inter-scale transfer term. However, in contrast to flows considered in previous studies, the local energy transfer is found to depend heavily on the linear contribution associated with the mean flow. Analysis of the scale-to-scale transfer of energy also allowed direct assessment of the classical picture of the energy cascade. It was found that while the inter-scale energy cascade driven by the turbulent fluctuations always proceeds in the forward direction, the total energy cascade driven by both the turbulent fluctuations and the mean flow exhibits significant inverse cascade regions, where energy is transferred from smaller to larger scales.

Turbulent flows
0022-1120
Knutsen, Anna N.
43be9178-2d54-4263-a7e4-1e77351b1062
Baj, Pawel
49fc4e45-ccba-4239-aca1-dd2ae896f0ca
Lawson, John M.
4e0b1895-51c5-41e6-9322-7f79e76e0e4c
Bodenschatz, Eberhard
e8658e96-6c7b-4385-94fa-a23fb68edeb5
Dawson, James R.
3dbd6c72-4af6-462d-aea3-11659ac6f095
Worth, Nicholas A.
87d86a76-3f9f-4ab9-bd4f-f091e7650d75
Knutsen, Anna N.
43be9178-2d54-4263-a7e4-1e77351b1062
Baj, Pawel
49fc4e45-ccba-4239-aca1-dd2ae896f0ca
Lawson, John M.
4e0b1895-51c5-41e6-9322-7f79e76e0e4c
Bodenschatz, Eberhard
e8658e96-6c7b-4385-94fa-a23fb68edeb5
Dawson, James R.
3dbd6c72-4af6-462d-aea3-11659ac6f095
Worth, Nicholas A.
87d86a76-3f9f-4ab9-bd4f-f091e7650d75

Knutsen, Anna N., Baj, Pawel, Lawson, John M., Bodenschatz, Eberhard, Dawson, James R. and Worth, Nicholas A. (2020) The inter-scale energy budget in a von Kármán mixing flow. Journal of Fluid Mechanics, 895, [A11]. (doi:10.1017/jfm.2020.277).

Record type: Article

Abstract

A detailed assessment of the inter-scale energy budget of the turbulent flow in a von Kármán mixing tank has been performed based on two extensive experimental data sets. Measurements were performed at a Taylor microscale Reynolds number of in the central region of the tank, using scanning particle image velocimetry (PIV) to fully resolve the velocity gradient tensor (VGT), and stereoscopic PIV for an expanded field of view. Following a basic flow characterisation, the Kármán-Howarth-Monin-Hill equation was used to investigate the inter-scale energy transfer. Access to the full VGT enabled the contribution of the different terms of the energy budget to be evaluated without any assumptions or approximations. The scale-space distribution of the dominant terms was also reported to assess the isotropy of the energy transfer. The results show a highly anisotropic distribution of energy transfer in scale space. Energy transfer was shown in a spherically averaged sense to be dominated at the small scales by the nonlinear inter-scale transfer term. However, in contrast to flows considered in previous studies, the local energy transfer is found to depend heavily on the linear contribution associated with the mean flow. Analysis of the scale-to-scale transfer of energy also allowed direct assessment of the classical picture of the energy cascade. It was found that while the inter-scale energy cascade driven by the turbulent fluctuations always proceeds in the forward direction, the total energy cascade driven by both the turbulent fluctuations and the mean flow exhibits significant inverse cascade regions, where energy is transferred from smaller to larger scales.

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More information

Accepted/In Press date: 8 April 2020
Published date: 18 May 2020
Additional Information: Funding Information: The authors gratefully acknowledge the support of the Max Planck Society and EuHIT: European High Performance Infrastructures in Turbulence, funded under the European Unions Seventh Framework Programme (FP7/2007-2013) grant agreement no. 312778. Publisher Copyright: © 2020 The Author(s). Published by Cambridge University Press. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.
Keywords: Turbulent flows

Identifiers

Local EPrints ID: 453371
URI: http://eprints.soton.ac.uk/id/eprint/453371
ISSN: 0022-1120
PURE UUID: e95e033e-02d0-4ec0-941f-dfc971f1a99b
ORCID for John M. Lawson: ORCID iD orcid.org/0000-0003-3260-3538

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Date deposited: 13 Jan 2022 18:16
Last modified: 18 Mar 2024 03:49

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Contributors

Author: Anna N. Knutsen
Author: Pawel Baj
Author: John M. Lawson ORCID iD
Author: Eberhard Bodenschatz
Author: James R. Dawson
Author: Nicholas A. Worth

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