Author:
Brandenburg Axel,Elstner Detlef,Masada Youhei,Pipin Valery
Abstract
AbstractMean-field dynamo theory has important applications in solar physics and galactic magnetism. We discuss some of the many turbulence effects relevant to the generation of large-scale magnetic fields in the solar convection zone. The mean-field description is then used to illustrate the physics of the $\alpha $
α
effect, turbulent pumping, turbulent magnetic diffusivity, and other effects on a modern solar dynamo model. We also discuss how turbulence transport coefficients are derived from local simulations of convection and then used in mean-field models.
Funder
Vetenskapsrådet
Ministry of Science and Higher Education of the Russian Federation
MEXT/JSPS KAKENHI
Central Research Institute of Stellar Explosive Phenomena (REISEP) at Fukuoka University
Stockholm University
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
5 articles.
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