2006/02/28 by P. J. Käpylä, M. J. Korpi, Mathieu Ossendrijver +2
Biochemistry, Genetics and Molecular Biology · Earth and Planetary Sciences · Mathematics · Physics and Astronomy · #Advection #Classical mechanics #Computational physics #Convection #Dynamo #Dynamo theory #Flux tube #Geomagnetism and Paleomagnetism Studies #Geometry #Geophysics and Gravity Measurements #Magnetic field #Magnetic flux #Magnetohydrodynamics #Mathematics #Mechanics #Physics #Quantum mechanics #Rotation (mathematics) #Solar and Space Plasma Dynamics #Turbulence #astro-ph
paper · pdf · doi:10.1051/0004-6361:20064972
published as Astron.Astrophys. 455 (2006) 401-412 · 14 pages, 12 figures, accepted for publication in Astronomy & Astrophysics
arxiv created 2006/05/10 · openalex publication_date 2006/08/01 · arxiv updated 2009/12/01 · openalex created_date 2022/08/01 · openalex updated_date 2026/08/05
Aims.The α- and γ-effects, which are responsible for the generation and turbulent pumping of large scale magnetic fields, respectively, due to passive advection by convection are determined in the rapid rotation regime corresponding to the deep layers of the solar convection zone.