Magnetic structures in a dynamo simulation

DOI10.1017/S0022112096001322zbMath0960.76540OpenAlexW2089961739MaRDI QIDQ4892855

R. L. Jennings, Ilkka Tuominen, Michel Rieutord, Åke Nordlund, Robert F. Stein, Axel Brandenburg

Publication date: 17 May 2001

Published in: Journal of Fluid Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1017/s0022112096001322

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05)

Related Items

Small-scale dynamo action in rotating compressible convection, On the nonlinear stability of the 1:1:1 ABC flow, The effect of time-dependentγ-pumping on buoyant magnetic structures, Stress-driven spin-down of a viscous fluid within a spherical shell, Magnetic-field generation and turbulence suppression due to cross-helicity effects, Coherent structures and the saturation of a nonlinear dynamo, Hydromagnetic turbulence in computer simulations, Direct numerical simulation of homogeneous stratified rotating turbulence, Fully developed turbulent dynamo at low magnetic Prandtl numbers, Fully developed turbulent dynamo at low magnetic Prandtl numbers, Dynamo in Asymmetric Square Convection, Oscillatory large-scale dynamos from Cartesian convection simulations, Dynamo efficiency in compressible convective dynamos with and without penetration

Cites Work

• 3-D simulations of solar and stellar convection and magnetoconvection
• What is a stellar dynamo?
• Models of intermittency in hydrodynamic turbulence