Bulletin of the American Physical Society
75th Annual Meeting of the Division of Fluid Dynamics
Volume 67, Number 19
Sunday–Tuesday, November 20–22, 2022; Indiana Convention Center, Indianapolis, Indiana.
Session Q21: Nonlinear Dynamics: Resolvents, Coherent Structures and Transition
1:25 PM–3:22 PM,
Monday, November 21, 2022
Room: 207
Chair: Robert Martinuzzi, University of Calgary
Abstract: Q21.00009 : Large-scale circulation patterns rule the predictability of extreme events*
3:09 PM–3:22 PM
Presenter:
Alberto Vela-Martin
(University of Bremen)
Authors:
Alberto Vela-Martin
(University of Bremen)
Marc Avila
(University of Bremen)
prediction is crucial to mitigate their consequences. Particularly now, in the context of climate change, interest has
emerged to develop models and indicators that allows for early detection and warning of extreme events. Some of these
models have proved successful, but it is unclear if they can be improved because the predictability limit of extreme
events is unknown. In this talk, we show that it is now possible to measure the predictability of extreme events directly by probing phase
space with a computationally-intensive approach. This allows to assess the exact potential of predictive models and to
determine precisely the conditions under which they may be effective. We analysed the predictability of extreme bursts
of the dissipation in a two-dimensional Kolmogorov flow by producing massive ensembles of initial conditions perturbed
around independent base flows. We produced millions of realisations to cover the full attractor of the Kolmogorov flow,
and used the Kullback—Leibler divergence, an information-theoretical tool, to assess predictability. This analysis
shows that extreme bursts of the dissipation may be successfully predicted beyond a few Lyapunov times, but that their
predictability depends strongly on the phase-space region from which they emerge. Specifically, we reveal that predictable
and unpredictable events evolve from two distinctly different large-scale circulation patterns. These results
open the possibility of improving predictive models by tuning them to the large-scale dynamics. Our approach could
be adapted with the available compute power to more complex flows.
*The authors acknowledge support from the Deutsche Forschungsgemeinschaft withinthe Priority Programme Turbulent Superstructures under Grant no. SPP 1881.
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