Skip to main navigation Skip to search Skip to main content

Nonlinear evolution of the horizontal shear instability in stratified rotating fluids under the complete Coriolis acceleration

  • Camille Moisset
  • , Paul Billant
  • , Junho Park
  • , Stéphane Mathis

Research output: Contribution to journalArticlepeer-review

Abstract

This paper investigates the nonlinear dynamics of horizontal shear instability in an incompressible, stratified and rotating fluid in the non-traditional $f$ -plane, i.e. with the full Coriolis acceleration, using direct numerical simulations. The study is restricted to two-dimensional horizontal perturbations. It is therefore independent of the vertical (traditional) Coriolis parameter. However, the flow has three velocity components due to the horizontal (non-traditional) Coriolis parameter. Three different scenarios of nonlinear evolution of the shear instability are identified, depending on the non-dimensional Brunt–Väisälä frequency $N$ and the non-dimensional non-traditional Coriolis parameter $\tilde {f}$ (non-dimensionalised by the maximum shear), in the range $\tilde {f}\lt N$ for fixed Reynolds and Schmidt numbers $ \textit{Re}=2000$ , $ \textit{Sc}=1$ . When the stratification is strong $N\gg 1$ , the shear instability generates stable Kelvin–Helmholtz billows like in the traditional limit $\tilde {f}=0$ . Furthermore, when $N\gg 1$ , the governing equations for any $\tilde {f}$ can be transformed into those for $\tilde {f}=0$ . This enables us to directly predict the characteristics of the flow depending on $\tilde {f}$ and $N$ . When $N$ is around unity and $\tilde {f}$ is above a threshold, the primary Kelvin–Helmholtz vortex is destabilised by secondary instabilities but it remains coherent. For weaker stratification, $N\leqslant 0.5$ and $\tilde {f}$ large enough, secondary instabilities develop vigorously and destroy the primary vortex into small-scales turbulence. Concomitantly, the enstrophy rises to high values by stretching/tilting as in fully three-dimensional flows. A local analysis of the flow prior to the onset of secondary instabilities reveals that the Fjørtoft necessary condition for instability is satisfied, suggesting that they correspond to shear instabilities.
Original languageEnglish
Article numberA28
Number of pages34
JournalJournal of Fluid Mechanics
Volume1027
Early online date19 Jan 2026
DOIs
Publication statusPublished - 25 Jan 2026

Funding

C.M. and S.M. acknowledge support from the European Research Council (ERC) under the Horizon Europe programme (Synergy grant agreement 101071505: 4D-STAR), from the CNES SOHO-GOLF and PLATO grants at CEA-DAp, and from PNP and PNPS (CNRS/INSU). While partially funded by the European Union, views and opinions expressed are, however, those of the authors only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. A part of this work was performed using HPC resources from GENCI-IDRIS (grant 2023- AD012A07419R2). The authors thank the referees for their detailed and constructive reports, which helpedthem to improve the article. We also thank F. Gallaire and A. Loyer for insightful discussions and V. Toai fortechnical assistance. C.M. and S.M. acknowledge support from the European Research Council (ERC) under the Horizon Europe programme (Synergy grant agreement 101071505: 4D-STAR), from the CNES SOHO-GOLF and PLATO grants at CEA-DAp, and from PNP and PNPS (CNRS/INSU). While partially funded by the European Union, views and opinions expressed are, however, those of the authors only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. A part of this work was performed using HPC resources from GENCI-IDRIS (grant 2023- AD012A07419R2). The authors thank the referees for their detailed and constructive reports, which helpedthem to improve the article. We also thank F. Gallaire and A. Loyer for insightful discussions and V. Toai fortechnical assistance.

FundersFunder number
European Research Council
Horizon Europe4D-STAR, 101071505
Grand Équipement National De Calcul Intensif2023- AD012A07419R2
Astrophysics Department, UMR AIM
CNRS Centre National de la Recherche Scientifique

    Keywords

    • geophysical and geological flows
    • instability
    • shear layers

    ASJC Scopus subject areas

    • Condensed Matter Physics
    • Mechanics of Materials
    • Mechanical Engineering
    • Applied Mathematics

    Fingerprint

    Dive into the research topics of 'Nonlinear evolution of the horizontal shear instability in stratified rotating fluids under the complete Coriolis acceleration'. Together they form a unique fingerprint.

    Cite this