Large-scale dynamos in turbulent convection with shear

2008/06/30 by P. J. Käpylä, M. J. Korpi, Axel Brandenburg +1 · 4 citations
Biochemistry, Genetics and Molecular Biology · Earth and Planetary Sciences · Physics and Astronomy · #Convection #Dynamo #Geology #Geomagnetism and Paleomagnetism Studies #Geophysics and Gravity Measurements #Magnetic field #Mechanics #Physics #Scale (ratio) #Shear (geology) #Solar and Space Plasma Dynamics #Turbulence #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810307

published as Astron. Astrophys. 491, 353-362 (2008) · 10 pages, 19 figures, accepted for publication in Astron. Astrophys

openalex publication_date 2008/10/03 · arxiv created 2008/10/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. To study the existence of large-scale convective dynamos under the influence of shear and rotation.

Citations

• Astrophysical magnetic fields and nonlinear dynamo theory
• The Case for a Distributed Solar Dynamo Shaped by Near‐Surface Shear
• Magnetoconvection and dynamo coefficients
• Local models of stellar convection:
• Magnetoconvection and dynamo coefficients:

Cited by

• Magnetorotational instability in a solar near-surface mean-field dynamo
• Interaction of Large- and Small-scale Dynamos in Isotropic Turbulent Flows from GPU-accelerated Simulations
• Large-scale dynamos in rapidly rotating plane layer convection
• Test-field method for mean-field coefficients with MHD background