Slow drift data of turbulent large-scale structures in axisymmetric co-rotating Taylor–Couette flow

DOI

Here we present data sets from direct numerical simulations of axisymmetric Taylor–Couette flow in the co-rotating regime that reveal a transition to spatio-temporal chaos as the system size increases. Beyond this transition, Taylor rolls suddenly undergo erratic drifts evolving on a very slow time scale. We estimate an effective diffusion coefficient for the drift and compare the dynamics to analogous motions in Rayleigh–Bénard convection and Poiseuille flow data sets, suggesting that this spontaneous diffusive displacement of large coherent structures is common among different types of wall-bounded turbulent flows.

Identifier
DOI https://doi.org/10.1594/PANGAEA.974809
Related Identifier IsSupplementTo https://doi.org/10.1017/jfm.2025.135
Metadata Access https://ws.pangaea.de/oai/provider?verb=GetRecord&metadataPrefix=datacite4&identifier=oai:pangaea.de:doi:10.1594/PANGAEA.974809
Provenance
Creator Feldmann, Daniel ORCID logo; Avila, Marc ORCID logo
Publisher PANGAEA
Publication Year 2025
Rights Creative Commons Attribution 4.0 International; https://creativecommons.org/licenses/by/4.0/
OpenAccess true
Representation
Resource Type Dataset
Format text/tab-separated-values
Size 45 data points
Discipline Earth System Research