Secondary instability, EOF reduction, and the transition to baroclinic chaos

DOI10.1016/0167-2789(94)00130-8zbMath0817.35080OpenAlexW2052468147MaRDI QIDQ1344776

Michael D. Mundt, John E. Hart

Publication date: 30 March 1995

Published in: Physica D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0167-2789(94)00130-8

zbMATH Keywords

numerical simulationsbaroclinic instabilityrotating stratified fluidsbifurcations to periodic and quasi-periodic statessymmetry-breaking secondary instabilities

Mathematics Subject Classification ID

PDEs in connection with fluid mechanics (35Q35) NLS equations (nonlinear Schrödinger equations) (35Q55) Dynamical systems approach to turbulence (76F20)

Related Items (2)

Reduced models of atmospheric low-frequency variability: parameter estimation and comparative performance ⋮ Symmetry and instability in rotating hydrodynamic and magnetohydrodynamic flows

Cites Work

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• Transition to time-dependent convection
• Recycling flow over bottom topography in a rotating annulus
• On the Stability of Two‐Dimensional Convection in a Layer Heated from Below
• The oscillatory instability of convection rolls in a low Prandtl number fluid
• A computational study of Rayleigh–Bénard convection. Part 2. Dimension considerations

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