Magnetic fields generated by hydromagnetic dynamos at the low Prandtl number in dependence on the Ekman and magnetic Prandtl numbers
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Physics and Astronomy (miscellaneous),Geophysics,Astronomy and Astrophysics
Reference33 articles.
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4. Remarks on some typical assumptions in dynamo theory;Busse;Geophys. Astrophys. Fluid Dyn.,2011
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1. Thermochemical convection in a slowly rotating spherical shell: a transition between prograde and retrograde flows;Geophysical & Astrophysical Fluid Dynamics;2024-03-03
2. Modelling convection-driven dynamo action in low-Prandtl-number fluids;Physica Scripta;2021-08-09
3. Transition from laminar to turbulent dynamo: the effect of varying Prandtl number;Geophysical & Astrophysical Fluid Dynamics;2020-08-20
4. Inertial effects on thermochemically driven convection and hydromagnetic dynamos in a spherical shell;Geophysical Journal International;2017-12-12
5. Magnetic and velocity fields in a dynamo operating at extremely small Ekman and magnetic Prandtl numbers;Contributions to Geophysics and Geodesy;2017-12-01
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