Wave interactions and the transition to chaos of baroclinic waves in a thermally driven rotating annulus
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Publication:3127906
DOI10.1098/rsta.1997.0003zbMath0875.76013OpenAlexW2041608056MaRDI QIDQ3127906
Publication date: 22 June 1997
Published in: Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1098/rsta.1997.0003
Experimental work for problems pertaining to fluid mechanics (76-05) General theory of rotating fluids (76U05)
Related Items (6)
Direct numerical simulation of transitions towards structural vacillation in an air-filled, rotating, baroclinic annulus ⋮ Mixed-mode solutions in an air-filled differentially heated rotating annulus ⋮ Flow transitions resembling bifurcations of the logistic map in simulations of the baroclinic rotating annulus ⋮ Onset of convection induced by centrifugal buoyancy in a rotating cavity ⋮ Spontaneous inertia–gravity wave emission in the differentially heated rotating annulus experiment ⋮ Instabilities and small-scale waves within the Stewartson layers of a thermally driven rotating annulus
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