Not much helicity is needed to drive large-scale dynamos

Understanding the in situ amplification of large-scale magnetic fields in turbulent astrophysical rotators has been a core subject of dynamo theory. When turbulent velocities are helical, large-scale dynamos that substantially amplify fields on scales that exceed the turbulent forcing scale arise, b...

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Guardado en:
Detalles Bibliográficos
Autor principal: Mininni, Pablo Daniel
Publicado: 2012
Materias:
Back reaction
Dynamo theories
Helicities
In-situ
Kinetic helicity
Magnetic spectra
Turbulent velocity
Wave numbers
Amplification
Astrophysics
Interactive devices
Magnetic fields
DC generators
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15393755_v85_n6_p_PietarilaGraham
http://hdl.handle.net/20.500.12110/paper_15393755_v85_n6_p_PietarilaGraham
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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