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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2. Steady and fluctuating inner core rotation in numerical geodynamo models;Aubert;Geophys. J. Int.,2011
3. Convection in rotating spherical fluid shells and its dynamo states;Busse,2005
4. Remarks on some typical assumptions in dynamo theory;Busse;Geophys. Astrophys. Fluid Dyn.,2011
5. Numerical modelling of the geodynamo: a systematic parameter study;Christensen;Geophys. J. Int.,1999
Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Modelling convection-driven dynamo action in low-Prandtl-number fluids;Physica Scripta;2021-08-09
2. Transition from laminar to turbulent dynamo: the effect of varying Prandtl number;Geophysical & Astrophysical Fluid Dynamics;2020-08-20
3. Inertial effects on thermochemically driven convection and hydromagnetic dynamos in a spherical shell;Geophysical Journal International;2017-12-12
4. Magnetic and velocity fields in a dynamo operating at extremely small Ekman and magnetic Prandtl numbers;Contributions to Geophysics and Geodesy;2017-12-01
5. Hydromagnetic dynamos at the low Ekman and magnetic Prandtl numbers;Contributions to Geophysics and Geodesy;2016-09-01
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