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Updated: Apr 5, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Stratification-Dependent Enstrophy-Controlled Regime in Geostrophic Turbulence
Shan-Shan Ding1, Hadrien Bobas2, Hélène Scolan3
1University of Oxford, Atmospheric, Oceanic and Planetary Physics, Department of Physics, OX1 3PU, United Kingdom.
Abstract:
We experimentally measure geostrophic turbulence in a rotating, differentially heated fluid annulus, which is bounded by convectively driven warm and cold flows at the outer and inner boundaries, respectively. The horizontal kinetic energy spectra exhibit a range at low wave number which scales as k^{-3}, where k denotes the horizontal wave number, with spectral amplitude that correlates with the square of the Brunt-Väisälä frequency at the same heights as the velocity measurements. The observed turbulent state exhibits a forward enstrophy cascade across all scales along with bidirectional energy transfer, which is evidenced by a reversal in the sign of the spectral energy flux at a scale proportional to the internal Rossby radius of deformation. These findings highlight the role of baroclinic instability in shaping the distribution of energy across scales, with implications for synoptic-scale turbulent flows near Earth's tropopause.
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