Direct simulations of helical Hall-MHD turbulence and dynamo action

Direct numerical simulations of turbulent Hall dynamos are presented. The evolution of an initially weak and small-scale magnetic field in a system maintained in a stationary turbulent regime by a stirring force at a macroscopic scale is studied to explore the conditions for exponential growth of th...

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Guardado en:
Detalles Bibliográficos
Publicado: 2005
Materias:
Accretion, accretion disks
Magnetic fields
MHD
Stars: magnetic fields
Stars: neutron
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v619_n2I_p1019_Mininni
http://hdl.handle.net/20.500.12110/paper_0004637X_v619_n2I_p1019_Mininni
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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