The fastest growing modes in rotating magnetoconvection with anisotropic diffusivities and their links to the Earth's core conditions
Author:
Affiliation:
1. Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia
2. ENEA, Italian National Agency for New Technologies, Energy and Sustainable Economic Development, Rome, Italy
Funder
Ministerstvo školstva, vedy, výskumu a športu Slovenskej republiky
Next Generation EU
Publisher
Informa UK Limited
Link
https://www.tandfonline.com/doi/pdf/10.1080/03091929.2024.2329552
Reference15 articles.
1. Local turbulence in the Earth's core
2. Braginsky S.I. and Roberts P.H. On the theory of convection in the Earth's core. In The Fluid Mechanics of Astrophysics and Geophysics Vol. 9 edited by A. Soward M.Ghil and P.H. Roberts pp. 60–82 2003 (Taylor and Francis group: London and New York).
3. Chandrasekhar, S., Hydrodynamic and Hydromagnetic Stability, 1961 (Clarendon Press: Oxford).
4. Cormier, V.F., Bergman, M.I. and Olson, P.L., Earth's Core: Geophysics of a Planet's Deepest Interior, 2022 (Amsterdam: Elsevier).
5. Cushman-Roisin, B., Introduction to Geophysical Fluid Dynamics, 1994 (Prentice Hall: Englewood Cliffs).
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1. Weakly nonlinear analysis of rotating magnetoconvection with anisotropic thermal diffusivity effect;Physics of Fluids;2024-07-01
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