Successive elimination of shear layers by a hierarchy of constraints in inviscid spherical-shell flows

DOI10.1063/1.4736990zbMath1277.76120OpenAlexW2057458507WikidataQ56837998 ScholiaQ56837998MaRDI QIDQ2865498

Philip W. Livermore, Rainer Hollerbach

Publication date: 29 November 2013

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.4736990

Mathematics Subject Classification ID

Shear flows and turbulence (76F10) General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (7)

The inherent instability of axisymmetric magnetostrophic dynamo models ⋮ Enumeration, orthogonality and completeness of the incompressible Coriolis modes in a sphere ⋮ On magnetostrophic dynamos in annular cores ⋮ The spherical harmonic spectrum of a function with algebraic singularities ⋮ Determination of the instantaneous geostrophic flow within the three-dimensional magnetostrophic regime ⋮ Electromagnetically driven zonal flows in a rapidly rotating spherical shell ⋮ On the equatorial Ekman layer

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• Imposing a magnetic field across a nonaxisymmetric shear layer in a rotating spherical shell
• The magneto-hydrodynamics of a rotating fluid and the earth’s dynamo problem
• On almost rigid rotations. Part 2

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