HEIndividual fellowship2023–2025

GeoCascade · Elucidating the bidirectional energy cascade of geophysical turbulence in time, space, and scale

Horizon Europe — Marie Skłodowska-Curie Actions

Duration
2023-09-18 → 2025-09-17
EU contribution
€181,153
Participants
2
Scheme
HORIZON-TMA-MSCA-PF-EF

Lines connect the coordinator with its partners.

Results in brief

Elucidating the bidirectional energy cascade of geophysical turbulence in time, space, and scale

Turbulence—the chaotic motion of fluids—governs how energy and momentum move through the atmosphere and oceans, shaping jets, storm tracks and mixing, and therefore affecting climate and extreme events. Because models cannot resolve all turbulent scales, they rely on closures built largely on idealised three dimensional turbulence, where energy cascades downscale. Real geophysical flows, however, are rotating, stratified and often confined in thin layers. Under these conditions, turbulence can split its energy simultaneously upscale and downscale (a bidirectional cascade), with a sharp onset as control parameters (e.g., rotation or aspect ratio) change. There is no quantitative theory for when this transition occurs, how the energy split depends on parameters, or which mechanisms drive it. This limits our ability to represent mixing, dissipation and the emergence of large scale structures in environmental models. This project set out to: (i) identify mechanisms responsible for the onset of bidirectional cascades; (ii) characterise their spatial and spectral signatures across scales; and (iii) develop a simple, quantitative model for the bidirectional cascade that can inform improved closures. Two complementary lenses were combined: - Spatial perspective: track how structures stretch, split, thin or merge across scales, to quantify their contributions to forward (downscale) and inverse (upscale) transfer. - Spectral perspective: analyse how interactions among Fourier modes depend on their phases; sustained flux requires phase organisation (“synchronisation”) across triads of interacting modes. High performance simulations (reduced “shell” models, two dimensional turbulence, and a large wall bounded flow used for a deviation study) enabled unprecedented sampling of noisy, nonlocal triad interactions, and provided the data needed to test theory. The key novelty is elevating triad phase dynamics from anecdotal evidence in extreme events to a predictive, scale by scale framework that links directly to energy flux. Pathway to impact: (a) open diagnostics and datasets to detect and quantify the balance between inverse and forward transfer; (b) theory informed parameterisations of energy flux direction and magnitude for weather, ocean and climate models; (c) practical guidance on when inverse cascade effects are expected and how to adjust closures; and (d) open source tools that lower the barrier to analysing cascade physics.

Data: CORDIS, © European Union

Project objective

Turbulent fluid motions are responsible for closing the energy budget in Earth’s atmosphere and on many astrophysical bodies, dictating their long-term evolution and climate. However, geophysical turbulence, even in the simplest contexts, remains an open problem. Past work has shown that the theory for homogeneous and isotropic turbulence (HIT) breaks down in a fluid subject to rotation, stratification, or large aspect ratios. Particularly affected is the central insight from the study of HIT, stating that energy moves to smaller scales through an ‘energy cascade’. In geophysical flows, energy can flow both to larger and smaller scales through a ‘bidirectional’ cascade. The fraction of energy going to large scales depends on the value of the relevant geophysical parameter, becoming nonzero at an apparent critical point. The goal of this project is to identify the spatial and spectral signatures of the bidirectional cascade, understand their role in the cascade’s sudden onset, and develop a quantitative theory for its subsequent development. We plan to use a combination of numerical and statistical methods to explore the bidirectional cascade in space, time, and scale. This analysis will be done through two complementary perspectives, investigating turbulent structures in physical space and in spectral space. In the former, the turbulent cascade manifests itself as individual structures which break up, merge, or clump together, depending on the regime. A statistical view of these interactions will provide insight on how the nature of the flow changes. On the other hand, in spectral space, the phases of the complex velocity amplitudes are known to be responsible for the exchange of energy among different length scales. We will look into a possible partial synchronization between these phases in our simulations, and attempt to model the transition to a bidirectional cascade using tools from the rich field of synchronization in complex networks.

Original text from CORDIS.

Participants

  • UNIVERSIDAD POLITECNICA DE MADRID · MadridCoordinatorSpain
  • UNIVERSITY COLLEGE DUBLIN, NATIONAL UNIVERSITY OF IRELAND, DUBLIN · DublinIreland

Links

Data: CORDIS, © European Union