Lack of universality in decaying magnetohydrodynamic turbulence

Autores
Lee, E.; Brachet, M. E.; Pouquet, A.; Mininni, Pablo Daniel; Rosenberg, Duane
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Using computations of three-dimensional magnetohydrodynamic (MHD) turbulence with a Taylor-Green flow, whose inherent time-independent symmetries are implemented numerically, and in the absence of either a forcing function or an imposed uniform magnetic field, we show that three different inertial ranges for the energy spectrum may emerge for three different initial magnetic fields, the selecting parameter being the ratio of nonlinear eddy to Alfvén time. Equivalent computational grids range from 1283 to 20483 points with a unit magnetic Prandtl number and a Taylor Reynolds number of up to 1500 at the peak of dissipation. We also show a convergence of our results with Reynolds number. Our study is consistent with previous findings of a variety of energy spectra in MHD turbulence by studies performed in the presence of both a forcing term with a given correlation time and a strong, uniform magnetic field. However, in contrast to the previous studies, here the ratio of characteristic time scales can only be ascribed to the intrinsic nonlinear dynamics of the paradigmatic flows under study. © 2010 The American Physical Society.
Fil: Lee, E.. Katholikie Universiteit Leuven; Bélgica. National Center for Atmospheric Research; Estados Unidos
Fil: Brachet, M. E.. National Center for Atmospheric Research; Estados Unidos. Ecole Normale Supérieure; Francia
Fil: Pouquet, A.. National Center for Atmospheric Research; Estados Unidos
Fil: Mininni, Pablo Daniel. National Center for Atmospheric Research; Estados Unidos. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Rosenberg, Duane. National Center for Atmospheric Research; Estados Unidos
Materia
Turbulent Flows
Magnetohydrodynamics And Electrohydrodynamics
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/59126

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spelling Lack of universality in decaying magnetohydrodynamic turbulenceLee, E.Brachet, M. E.Pouquet, A.Mininni, Pablo DanielRosenberg, DuaneTurbulent FlowsMagnetohydrodynamics And Electrohydrodynamicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using computations of three-dimensional magnetohydrodynamic (MHD) turbulence with a Taylor-Green flow, whose inherent time-independent symmetries are implemented numerically, and in the absence of either a forcing function or an imposed uniform magnetic field, we show that three different inertial ranges for the energy spectrum may emerge for three different initial magnetic fields, the selecting parameter being the ratio of nonlinear eddy to Alfvén time. Equivalent computational grids range from 1283 to 20483 points with a unit magnetic Prandtl number and a Taylor Reynolds number of up to 1500 at the peak of dissipation. We also show a convergence of our results with Reynolds number. Our study is consistent with previous findings of a variety of energy spectra in MHD turbulence by studies performed in the presence of both a forcing term with a given correlation time and a strong, uniform magnetic field. However, in contrast to the previous studies, here the ratio of characteristic time scales can only be ascribed to the intrinsic nonlinear dynamics of the paradigmatic flows under study. © 2010 The American Physical Society.Fil: Lee, E.. Katholikie Universiteit Leuven; Bélgica. National Center for Atmospheric Research; Estados UnidosFil: Brachet, M. E.. National Center for Atmospheric Research; Estados Unidos. Ecole Normale Supérieure; FranciaFil: Pouquet, A.. National Center for Atmospheric Research; Estados UnidosFil: Mininni, Pablo Daniel. National Center for Atmospheric Research; Estados Unidos. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Rosenberg, Duane. National Center for Atmospheric Research; Estados UnidosAmerican Physical Society2010-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/59126Lee, E.; Brachet, M. E.; Pouquet, A.; Mininni, Pablo Daniel; Rosenberg, Duane; Lack of universality in decaying magnetohydrodynamic turbulence; American Physical Society; Physical Review E: Statistical, Nonlinear and Soft Matter Physics; 81; 1; 1-2010; 163181-1631891539-3755CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevE.81.016318info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-10T13:13:38Zoai:ri.conicet.gov.ar:11336/59126instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-10 13:13:38.508CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Lack of universality in decaying magnetohydrodynamic turbulence
title Lack of universality in decaying magnetohydrodynamic turbulence
spellingShingle Lack of universality in decaying magnetohydrodynamic turbulence
Lee, E.
Turbulent Flows
Magnetohydrodynamics And Electrohydrodynamics
title_short Lack of universality in decaying magnetohydrodynamic turbulence
title_full Lack of universality in decaying magnetohydrodynamic turbulence
title_fullStr Lack of universality in decaying magnetohydrodynamic turbulence
title_full_unstemmed Lack of universality in decaying magnetohydrodynamic turbulence
title_sort Lack of universality in decaying magnetohydrodynamic turbulence
dc.creator.none.fl_str_mv Lee, E.
Brachet, M. E.
Pouquet, A.
Mininni, Pablo Daniel
Rosenberg, Duane
author Lee, E.
author_facet Lee, E.
Brachet, M. E.
Pouquet, A.
Mininni, Pablo Daniel
Rosenberg, Duane
author_role author
author2 Brachet, M. E.
Pouquet, A.
Mininni, Pablo Daniel
Rosenberg, Duane
author2_role author
author
author
author
dc.subject.none.fl_str_mv Turbulent Flows
Magnetohydrodynamics And Electrohydrodynamics
topic Turbulent Flows
Magnetohydrodynamics And Electrohydrodynamics
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Using computations of three-dimensional magnetohydrodynamic (MHD) turbulence with a Taylor-Green flow, whose inherent time-independent symmetries are implemented numerically, and in the absence of either a forcing function or an imposed uniform magnetic field, we show that three different inertial ranges for the energy spectrum may emerge for three different initial magnetic fields, the selecting parameter being the ratio of nonlinear eddy to Alfvén time. Equivalent computational grids range from 1283 to 20483 points with a unit magnetic Prandtl number and a Taylor Reynolds number of up to 1500 at the peak of dissipation. We also show a convergence of our results with Reynolds number. Our study is consistent with previous findings of a variety of energy spectra in MHD turbulence by studies performed in the presence of both a forcing term with a given correlation time and a strong, uniform magnetic field. However, in contrast to the previous studies, here the ratio of characteristic time scales can only be ascribed to the intrinsic nonlinear dynamics of the paradigmatic flows under study. © 2010 The American Physical Society.
Fil: Lee, E.. Katholikie Universiteit Leuven; Bélgica. National Center for Atmospheric Research; Estados Unidos
Fil: Brachet, M. E.. National Center for Atmospheric Research; Estados Unidos. Ecole Normale Supérieure; Francia
Fil: Pouquet, A.. National Center for Atmospheric Research; Estados Unidos
Fil: Mininni, Pablo Daniel. National Center for Atmospheric Research; Estados Unidos. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Rosenberg, Duane. National Center for Atmospheric Research; Estados Unidos
description Using computations of three-dimensional magnetohydrodynamic (MHD) turbulence with a Taylor-Green flow, whose inherent time-independent symmetries are implemented numerically, and in the absence of either a forcing function or an imposed uniform magnetic field, we show that three different inertial ranges for the energy spectrum may emerge for three different initial magnetic fields, the selecting parameter being the ratio of nonlinear eddy to Alfvén time. Equivalent computational grids range from 1283 to 20483 points with a unit magnetic Prandtl number and a Taylor Reynolds number of up to 1500 at the peak of dissipation. We also show a convergence of our results with Reynolds number. Our study is consistent with previous findings of a variety of energy spectra in MHD turbulence by studies performed in the presence of both a forcing term with a given correlation time and a strong, uniform magnetic field. However, in contrast to the previous studies, here the ratio of characteristic time scales can only be ascribed to the intrinsic nonlinear dynamics of the paradigmatic flows under study. © 2010 The American Physical Society.
publishDate 2010
dc.date.none.fl_str_mv 2010-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/59126
Lee, E.; Brachet, M. E.; Pouquet, A.; Mininni, Pablo Daniel; Rosenberg, Duane; Lack of universality in decaying magnetohydrodynamic turbulence; American Physical Society; Physical Review E: Statistical, Nonlinear and Soft Matter Physics; 81; 1; 1-2010; 163181-163189
1539-3755
CONICET Digital
CONICET
url http://hdl.handle.net/11336/59126
identifier_str_mv Lee, E.; Brachet, M. E.; Pouquet, A.; Mininni, Pablo Daniel; Rosenberg, Duane; Lack of universality in decaying magnetohydrodynamic turbulence; American Physical Society; Physical Review E: Statistical, Nonlinear and Soft Matter Physics; 81; 1; 1-2010; 163181-163189
1539-3755
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevE.81.016318
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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