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On the origin of frequency sparsity in direct numerical simulations of turbulent pipe flow

On the origin of frequency sparsity in direct numerical simulations of turbulent pipe flow
On the origin of frequency sparsity in direct numerical simulations of turbulent pipe flow
The possibility of creating reduced-order models for canonical wall-bounded turbulent flows based on exploiting energy sparsity in frequency domain, as proposed by Bourguignon et al. [Phys. Fluids26, 015109 (2014)], is examined. The present letter explains the origins of energetically sparse dominant frequencies and provides fundamental information for the design of such reduced-order models. The resolvent decomposition of a pipe flow is employed to consider the influence of finite domain length on the flow dynamics, which acts as a restriction on the possible wavespeeds in the flow. A forcing-to-fluctuation gain analysis in the frequency domain reveals that large sparse peaks in amplification occur when one of the possible wavespeeds matches the local wavespeed via the critical layer mechanism. A link between amplification and energy is provided through the similar characteristics exhibited by the most energetically relevant flow structures, arising from a dynamic mode decomposition of direct numerical simulation data, and the resolvent modes associated with the most amplified sparse frequencies. These results support the feasibility of reduced-order models based on the selection of the most amplified modes emerging from the resolvent model, leading to a novel computationally efficient method of representing turbulent flows.
1070-6631
101703-[8pp]
Gomez, F.
3cd7f89a-64df-4c02-b5c5-f6823cdf3180
Blackburn, H.M
02b68907-6382-448e-a6a1-d111c514fd54
Rudman, M.
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McKeon, B.J.
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Luhar, M.
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Moarref, R.
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Sharma, A.S.
cdd9deae-6f3a-40d9-864c-76baf85d8718
Gomez, F.
3cd7f89a-64df-4c02-b5c5-f6823cdf3180
Blackburn, H.M
02b68907-6382-448e-a6a1-d111c514fd54
Rudman, M.
1eb7fd54-c427-416e-9e5b-2f548ae0b5b5
McKeon, B.J.
2e685015-292a-42a7-8c9e-7cc27cf2da67
Luhar, M.
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Moarref, R.
5f671bcc-1836-4642-a2f9-c9f122e8477c
Sharma, A.S.
cdd9deae-6f3a-40d9-864c-76baf85d8718

Gomez, F., Blackburn, H.M, Rudman, M., McKeon, B.J., Luhar, M., Moarref, R. and Sharma, A.S. (2014) On the origin of frequency sparsity in direct numerical simulations of turbulent pipe flow. Physics of Fluids, 26 (10), 101703-[8pp]. (doi:10.1063/1.4900768).

Record type: Article

Abstract

The possibility of creating reduced-order models for canonical wall-bounded turbulent flows based on exploiting energy sparsity in frequency domain, as proposed by Bourguignon et al. [Phys. Fluids26, 015109 (2014)], is examined. The present letter explains the origins of energetically sparse dominant frequencies and provides fundamental information for the design of such reduced-order models. The resolvent decomposition of a pipe flow is employed to consider the influence of finite domain length on the flow dynamics, which acts as a restriction on the possible wavespeeds in the flow. A forcing-to-fluctuation gain analysis in the frequency domain reveals that large sparse peaks in amplification occur when one of the possible wavespeeds matches the local wavespeed via the critical layer mechanism. A link between amplification and energy is provided through the similar characteristics exhibited by the most energetically relevant flow structures, arising from a dynamic mode decomposition of direct numerical simulation data, and the resolvent modes associated with the most amplified sparse frequencies. These results support the feasibility of reduced-order models based on the selection of the most amplified modes emerging from the resolvent model, leading to a novel computationally efficient method of representing turbulent flows.

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Published date: 31 October 2014
Organisations: Aerodynamics & Flight Mechanics Group

Identifiers

Local EPrints ID: 370686
URI: http://eprints.soton.ac.uk/id/eprint/370686
ISSN: 1070-6631
PURE UUID: 58e9e9a6-184f-46da-9aa7-f1873d2fdaee
ORCID for A.S. Sharma: ORCID iD orcid.org/0000-0002-7170-1627

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Date deposited: 04 Nov 2014 09:45
Last modified: 15 Mar 2024 03:46

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Contributors

Author: F. Gomez
Author: H.M Blackburn
Author: M. Rudman
Author: B.J. McKeon
Author: M. Luhar
Author: R. Moarref
Author: A.S. Sharma ORCID iD

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