Magnetohydrodynamics of stably stratified regions in planets and stars
DOI10.1080/03091929.2019.1670827zbMath1482.76147arXiv1910.04092OpenAlexW3100888701WikidataQ114640042 ScholiaQ114640042MaRDI QIDQ5065683
C. Gissinger, J. Philidet, François Lignières, Ludovic Petitdemange
Publication date: 22 March 2022
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1910.04092
direct numerical simulationsouter coreEarth: stably stratified layermagnetic desertstars: radiative zones
Direct numerical and large eddy simulation of turbulence (76F65) Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Cites Work
- Spherical Couette flow in a dipolar magnetic field
- Experimental study of super-rotation in a magnetostrophic spherical Couette flow
- Mathematical Aspects of Natural Dynamos
- A super-rotating shear layer in magnetohydrodynamic spherical Couette flow
- On the steady motions produced by a stable stratification in a rapidly rotating fluid
- Linear theory of rotating stratified fluid motions
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