On magnetostrophic inertia-less waves in quasi-geostrophic models of planetary cores

DOI10.1080/03091929.2015.1094569OpenAlexW1820374732WikidataQ114640168 ScholiaQ114640168MaRDI QIDQ5879702

F. Labbé, D. Jault, N. Gillet

Publication date: 2 March 2023

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091929.2015.1094569

zbMATH Keywords

magnetostrophic wavesTaylor's constrainttorsional wavesquasi-geostrophy

Mathematics Subject Classification ID

General and overarching topics; collections (00-XX)

Related Items (6)

Could hydrodynamic Rossby waves explain the westward drift? ⋮ Characterization of columnar inertial modes in rapidly rotating spheres and spheroids ⋮ Plesio-geostrophy for Earth’s core: I. Basic equations, inertial modes and induction ⋮ Subcritical convection of liquid metals in a rotating sphere using a quasi-geostrophic model ⋮ Compressible fluid modes in rigid ellipsoids: towards modal acoustic velocimetry ⋮ Mean zonal flows induced by weak mechanical forcings in rotating spheroids

Cites Work

• On inertial waves in a rotating fluid sphere
• Deep two-dimensional turbulence: An idealized model for atmospheric jets of the giant outer planets
• Quasigeostrophic model of the instabilities of the Stewartson layer in flat and depth-varying containers
• The magneto-hydrodynamics of a rotating fluid and the earth’s dynamo problem
• The quasi-geostrophic model for rapidly rotating spherical convection outside the tangent cylinder
• Hydromagnetic planetary waves
• On hydromagnetic oscillations in a rotating cavity
• On the theory of core-mantle coupling
• On magnetostrophic mean-field solutions of the geodynamo equations

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