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Kranz, Felix (2025): A dataset of energy-optimal driving waveforms in turbulent pipe flow [dataset]. PANGAEA, https://doi.org/10.1594/PANGAEA.986097

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Published: 2025-10-20DOI registered: 2025-11-19

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Abstract:
We compute drag- and energy-optimal driving waveforms in turbulent pipe flow using direct numerical simulations combined with a gradient-free, black-box optimisation framework. Our results demonstrate that Bayesian optimisation significantly outperforms conventional gradient-based methods in terms of efficiency and robustness, owing to its ability to handle noisy objective functions that arise from the finite-time averaging of turbulent flows. Optimal waveforms are identified for three Reynolds numbers and two Womersley numbers. At a Reynolds number of 8600 and a Womersley number of 10, the optimal waveforms reduce total energy consumption by up to 22% and drag by up to 37%. This dataset includes the optimal waveforms, instantaneous and time-averaged velocity fields, as well as post-processing scripts.
Keyword(s):
drag reduction; turbulence control; turbulent pipe flow
Related to:
Morón, Daniel; Avila, Marc: Bayesian minimisation of energy consumption in turbulent pipe flow via unsteady driving. https://arxiv.org/pdf/2508.14593
Parameter(s):
#NameShort NameUnitPrincipal InvestigatorMethod/DeviceComment
Binary ObjectBinaryKranz, FelixNumerical simulated
Binary Object (File Size)Binary (Size)BytesKranz, FelixNumerical simulated
FigureFigKranz, FelixNumerical simulated
TitleTitleKranz, FelixNumerical simulated
File nameFile nameKranz, FelixNumerical simulated
VariableVariableKranz, FelixNumerical simulated
Status:
Curation Level: Enhanced curation (CurationLevelC) * Processing Level: PANGAEA data processing level 2 (ProcLevel2)
Size:
59 data points

Data

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Variable
fig1.zip279.2 MBytes1(a) Schematic description of the considered triangular waveforms in terms of the time variant Reynolds number or bulk velocity. (b) The evolution of the volume-integrated cross-stream turbulent kinetic energy. (c) The wall shear stress and power input over the last three periods of a four period run driven in the same manner as in (a).fig1.zipPython scripts to produce figure 1 along with .pkl files containing the underlying data
fig2.zip538.2 kBytes2(a) The relative standard error of the per-period wall shear stress versus the number of averaging periods. (b) The computational time to achieve a given standard error.fig2.zipPython scripts to produce figure 2 along with .pkl files containing the underlying data
fig3.zip850.8 kBytes3Best surrogates for the mean wall shear stress and power inputfig3.zipPython scripts to produce figure 3 along with .pkl files containing the underlying data
fig4.zip31.7 MBytes4Optimal triangular waveforms at Re=5160fig4.zipPython scripts to produce figure 4 along with .pkl files containing the underlying data
fig5.zip568.1 kBytes5Partial dependence for the wall stress and power input on acceleration time, minimum Reynolds number and maximum Reynolds numberfig5.zipPython scripts to produce figure 5 along with .pkl files containing the underlying data
fig6.zip92.8 MBytes6Power-optimal waveforms obtained from three independent runs of the truncated Fourier approach at Re=5160 and Wo=10fig6.zipPython scripts to produce figure 6 along with .pkl files containing the underlying data
fig7.zip152 MBytes7Power-optimal waveform at Re=8600 and Wo=10fig7.zipPython scripts to produce figure 7 along with .pkl files containing the underlying data
fig8_9_13_14.zip49.9 GBytes8,9,13,14Time evolution of dissipation, production, spatial wall-shear stress distribution and turbulent kinetic energy for a (sub-)optimal waveformfig8_9_13_14.zipPython scripts to produce figure 8, 9, 13, 14 along with .pkl files containing the underlying data
fig10.zip627.1 kBytes10The evolution of the optimisation process for different choices of the admissible standard errorfig10.zipPython scripts to produce figure 10 along with .pkl files containing the underlying data
fig11.zip12.5 MBytes11The power-optimal waveform obtained at Wo=10*2^0.5fig11.zipPython scripts to produce figure 11 along with .pkl files containing the underlying data
fig12.zip135 MBytes12The evolution of the turbulent kinetic energy for waveforms 1-3 without forcing termfig12.zipPython scripts to produce figure 12 along with .pkl files containing the underlying data
utils.zip15 kBytesPython scripts required to run the aboveutils.zipPython scripts required to run the above