Direct numerical simulations of helical dynamo action: MHD and beyond

Magnetohydrodynamic dynamo action is often invoked to explain the existence of magnetic fields in several astronomical objects. In this work, we present direct numerical simulations of MHD helical dynamos, to study the exponential growth and saturation of magnetic fields. Simulations are made within...

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Autores principales: Gómez, D.O., Mininni, P.D.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_10235809_v11_n5-6_p619_Gomez
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spelling todo:paper_10235809_v11_n5-6_p619_Gomez2023-10-03T15:56:48Z Direct numerical simulations of helical dynamo action: MHD and beyond Gómez, D.O. Mininni, P.D. magnetohydrodynamics numerical model Magnetohydrodynamic dynamo action is often invoked to explain the existence of magnetic fields in several astronomical objects. In this work, we present direct numerical simulations of MHD helical dynamos, to study the exponential growth and saturation of magnetic fields. Simulations are made within the framework of incompressible flows and using periodic boundary conditions. The statistical properties of the flow are studied, and it is found that its helicity displays strong spatial fluctuations. Regions with large kinetic helicity are also strongly concentrated in space, forming elongated structures. In dynamo simulations using these flows, we found that the growth rate and the saturation level of magnetic energy and magnetic helicity reach an asymptotic value as the Reynolds number is increased. Finally, extensions of the MHD theory to include kinetic effects relevant in astrophysical environments are discussed. © European Geosciences Union 2004. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_10235809_v11_n5-6_p619_Gomez
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic magnetohydrodynamics
numerical model
spellingShingle magnetohydrodynamics
numerical model
Gómez, D.O.
Mininni, P.D.
Direct numerical simulations of helical dynamo action: MHD and beyond
topic_facet magnetohydrodynamics
numerical model
description Magnetohydrodynamic dynamo action is often invoked to explain the existence of magnetic fields in several astronomical objects. In this work, we present direct numerical simulations of MHD helical dynamos, to study the exponential growth and saturation of magnetic fields. Simulations are made within the framework of incompressible flows and using periodic boundary conditions. The statistical properties of the flow are studied, and it is found that its helicity displays strong spatial fluctuations. Regions with large kinetic helicity are also strongly concentrated in space, forming elongated structures. In dynamo simulations using these flows, we found that the growth rate and the saturation level of magnetic energy and magnetic helicity reach an asymptotic value as the Reynolds number is increased. Finally, extensions of the MHD theory to include kinetic effects relevant in astrophysical environments are discussed. © European Geosciences Union 2004.
format JOUR
author Gómez, D.O.
Mininni, P.D.
author_facet Gómez, D.O.
Mininni, P.D.
author_sort Gómez, D.O.
title Direct numerical simulations of helical dynamo action: MHD and beyond
title_short Direct numerical simulations of helical dynamo action: MHD and beyond
title_full Direct numerical simulations of helical dynamo action: MHD and beyond
title_fullStr Direct numerical simulations of helical dynamo action: MHD and beyond
title_full_unstemmed Direct numerical simulations of helical dynamo action: MHD and beyond
title_sort direct numerical simulations of helical dynamo action: mhd and beyond
url http://hdl.handle.net/20.500.12110/paper_10235809_v11_n5-6_p619_Gomez
work_keys_str_mv AT gomezdo directnumericalsimulationsofhelicaldynamoactionmhdandbeyond
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