Direct numerical simulation of transitions towards structural vacillation in an air-filled, rotating, baroclinic annulus
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Publication:5303898
DOI10.1063/1.2911045zbMath1182.76622OpenAlexW2083404885MaRDI QIDQ5303898
Pierre Maubert, P. L. Read, Wolf-Gerrit Früh, Anthony Randriamampianina
Publication date: 18 March 2010
Published in: Physics of Fluids (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.2911045
chaosconvectionturbulencecomputational fluid dynamicsnumerical analysisflow instabilityfluid oscillationsstratified flowrotational flow
Related Items (4)
Coriolis effect on centrifugal buoyancy-driven convection in a thin cylindrical shell ⋮ The primary flow transition in a differentially heated rotating channel of fluid with \(\mathrm{O}(2)\) symmetry ⋮ Onset of convection induced by centrifugal buoyancy in a rotating cavity ⋮ Instabilities and small-scale waves within the Stewartson layers of a thermally driven rotating annulus
Cites Work
- Transition to geostrophic turbulence in an air-filled differentially heated rotating annulus
- Determining Lyapunov exponents from a time series
- Phase portrait reconstruction using multivariate singular systems analysis
- A spectral projection method for the simulation of complex three-dimensional rotating flows
- Linear stability analysis for the differentially heated rotating annulus
- Wave interactions and the transition to chaos of baroclinic waves in a thermally driven rotating annulus
- Continuation of travelling-wave solutions of the Navier–Stokes equations
- Convection in a rotating cylindrical annulus: thermal Rossby waves
- Convection in a rotating cylindrical annulus. Part 2. Transitions to asymmetric and vacillating flow
- Convection in a rotating cylindrical annulus Part 3. Vacillating and spatially modulated flows
- Double Hopf Bifurcations in the Differentially Heated Rotating Annulus
- Convection induced by centrifugal buoyancy
- Direct numerical simulations of bifurcations in an air-filled rotating baroclinic annulus
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