TY - JOUR
T1 - Nonlinear evolution of the horizontal shear instability in stratified rotating fluids under the complete Coriolis acceleration
AU - Moisset, Camille
AU - Billant, Paul
AU - Park, Junho
AU - Mathis, Stéphane
PY - 2026/1/25
Y1 - 2026/1/25
N2 - 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.
AB - 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.
KW - geophysical and geological flows
KW - instability
KW - shear layers
UR - https://www.scopus.com/pages/publications/105028436906
U2 - 10.1017/jfm.2025.11072
DO - 10.1017/jfm.2025.11072
M3 - Article
SN - 0022-1120
VL - 1027
JO - Journal of Fluid Mechanics
JF - Journal of Fluid Mechanics
M1 - A28
ER -