Probing turbulent superstructures in Rayleigh-B\'{e}nard convection by Lagrangian trajectory clusters
Christiane Schneide, Ambrish Pandey, Kathrin Padberg-Gehle, and J\"org, Schumacher

TL;DR
This paper uses Lagrangian trajectory clustering to identify and analyze large-scale turbulent superstructures in Rayleigh-Bénard convection, demonstrating the method's effectiveness and consistency with Eulerian measures.
Contribution
It introduces a trajectory clustering approach based on graph Laplacian spectra to detect turbulent superstructures, extending analysis to longer times with density-based clustering.
Findings
Trajectory clusters match Eulerian superstructures.
Lagrangian and Eulerian characteristic times and lengths agree.
Longer times require density-based clustering for coherent structures.
Abstract
We analyze large-scale patterns in three-dimensional turbulent convection in a horizontally extended square convection cell by Lagrangian particle trajectories calculated in direct numerical simulations. A simulation run at a Prandtl number Pr , a Rayleigh number Ra , and an aspect ratio is therefore considered. These large-scale structures, which are denoted as turbulent superstructures of convection, are detected by the spectrum of the graph Laplacian matrix. Our investigation, which follows Hadjighasem {\it et al.}, Phys. Rev. E {\bf 93}, 063107 (2016), builds a weighted and undirected graph from the trajectory points of Lagrangian particles. Weights at the edges of the graph are determined by a mean dynamical distance between different particle trajectories. It is demonstrated that the resulting trajectory clusters, which are obtained by a subsequent…
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