Convection-driven kinematic dynamos with a self-consistent shear flow

DOI10.1080/03091929.2018.1517210OpenAlexW3098598520WikidataQ114640083 ScholiaQ114640083MaRDI QIDQ5063547

L. K. Currie, S. M. Tobias

Publication date: 21 March 2022

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

Full work available at URL: https://arxiv.org/abs/1811.12737

zbMATH Keywords

convectionsheardynamos

Mathematics Subject Classification ID

Fluid mechanics (76-XX) Astronomy and astrophysics (85-XX)

Uses Software

• ASCL
• Dedalus

Cites Work

• Unnamed Item
• Rigorous bounds on the fast dynamo growth rate involving topological entropy
• Kinematic dynamo action in large magnetic Reynolds number flows driven by shear and convection
• The shear dynamo problem for small magnetic Reynolds numbers
• Dynamo action in complex flows: the quick and the fast
• Mathematical Aspects of Natural Dynamos
• Three-dimensional simulations of convection in layers with tilted rotation vectors
• Convective instability when the temperature gradient and rotation vector are oblique to gravity. II. Real fluids with effects of diffusion
• Strongly nonlinear convection cells in a rapidly rotating fluid layer: the tilted f-plane
• Magnetic field generation by the motion of a highly conducting fluid
• The Magnetic Field of Sunspots
• Stretch, Twist, Fold: The Fast Dynamo
• Dynamo action in a rotating convective layer
• The α-chain-termination mutants and their relation to the α-thalassaemias

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