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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/59126
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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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1842980722665586688 |
score |
12.993085 |