Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind

Autores
Greco, Andres Francisco; Servidio, S.; Matthaeus, W.H.; Dmitruk, Pablo Ariel
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this work we review some recent studies, in which properties of the magnetic field in high resolution simulations of MHD turbulence with spacecraft data are compared, focusing on methods used to identify classical discontinuities and intermittency statistics. Comparison of ACE solar wind data and simulations of MHD turbulence showed good agreement in waiting-time analysis of magnetic discontinuities, and in the related distribution of magnetic field increments. Further analyses showed that the magnetic discontinuities are not distributed without correlations, but rather that non-Poisson correlations, possibly in the form of burstiness or voids, are present in the data at least up to the typical correlation scale. The discontinuities or bursty coherent structures represent in this view the current sheets that form between magnetic flux tubes which may be a signature of intermittent, anisotropic, fully developed MHD turbulence. © 2010 Elsevier Ltd. All rights reserved. All rights reserved.
Fil: Greco, Andres Francisco. 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: Servidio, S.. Universita Della Calabria;
Fil: Matthaeus, W.H.. Bartol Research Institute;
Fil: Dmitruk, Pablo Ariel. 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
Materia
Intermittency
Magnetic Discontinuities
Mhd Simulations
Solar Wind
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:11336/57201
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/57201
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar windGreco, Andres FranciscoServidio, S.Matthaeus, W.H.Dmitruk, Pablo ArielIntermittencyMagnetic DiscontinuitiesMhd SimulationsSolar Windhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work we review some recent studies, in which properties of the magnetic field in high resolution simulations of MHD turbulence with spacecraft data are compared, focusing on methods used to identify classical discontinuities and intermittency statistics. Comparison of ACE solar wind data and simulations of MHD turbulence showed good agreement in waiting-time analysis of magnetic discontinuities, and in the related distribution of magnetic field increments. Further analyses showed that the magnetic discontinuities are not distributed without correlations, but rather that non-Poisson correlations, possibly in the form of burstiness or voids, are present in the data at least up to the typical correlation scale. The discontinuities or bursty coherent structures represent in this view the current sheets that form between magnetic flux tubes which may be a signature of intermittent, anisotropic, fully developed MHD turbulence. © 2010 Elsevier Ltd. All rights reserved. All rights reserved.Fil: Greco, Andres Francisco. 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: Servidio, S.. Universita Della Calabria;Fil: Matthaeus, W.H.. Bartol Research Institute;Fil: Dmitruk, Pablo Ariel. 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; ArgentinaPergamon-Elsevier Science Ltd2010-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/57201Greco, Andres Francisco; Servidio, S.; Matthaeus, W.H.; Dmitruk, Pablo Ariel; Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind; Pergamon-Elsevier Science Ltd; Planetary and Space Science; 58; 14-15; 12-2010; 1895-18990032-0633CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.pss.2010.08.019info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:24:53Zoai:ri.conicet.gov.ar:11336/57201instacron: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:34982025-10-15 14:24:53.826CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
title Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
spellingShingle Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
Greco, Andres Francisco
Intermittency
Magnetic Discontinuities
Mhd Simulations
Solar Wind
title_short Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
title_full Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
title_fullStr Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
title_full_unstemmed Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
title_sort Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind
dc.creator.none.fl_str_mv Greco, Andres Francisco
Servidio, S.
Matthaeus, W.H.
Dmitruk, Pablo Ariel
author Greco, Andres Francisco
author_facet Greco, Andres Francisco
Servidio, S.
Matthaeus, W.H.
Dmitruk, Pablo Ariel
author_role author
author2 Servidio, S.
Matthaeus, W.H.
Dmitruk, Pablo Ariel
author2_role author
author
author
dc.subject.none.fl_str_mv Intermittency
Magnetic Discontinuities
Mhd Simulations
Solar Wind
topic Intermittency
Magnetic Discontinuities
Mhd Simulations
Solar Wind
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this work we review some recent studies, in which properties of the magnetic field in high resolution simulations of MHD turbulence with spacecraft data are compared, focusing on methods used to identify classical discontinuities and intermittency statistics. Comparison of ACE solar wind data and simulations of MHD turbulence showed good agreement in waiting-time analysis of magnetic discontinuities, and in the related distribution of magnetic field increments. Further analyses showed that the magnetic discontinuities are not distributed without correlations, but rather that non-Poisson correlations, possibly in the form of burstiness or voids, are present in the data at least up to the typical correlation scale. The discontinuities or bursty coherent structures represent in this view the current sheets that form between magnetic flux tubes which may be a signature of intermittent, anisotropic, fully developed MHD turbulence. © 2010 Elsevier Ltd. All rights reserved. All rights reserved.
Fil: Greco, Andres Francisco. 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: Servidio, S.. Universita Della Calabria;
Fil: Matthaeus, W.H.. Bartol Research Institute;
Fil: Dmitruk, Pablo Ariel. 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
description In this work we review some recent studies, in which properties of the magnetic field in high resolution simulations of MHD turbulence with spacecraft data are compared, focusing on methods used to identify classical discontinuities and intermittency statistics. Comparison of ACE solar wind data and simulations of MHD turbulence showed good agreement in waiting-time analysis of magnetic discontinuities, and in the related distribution of magnetic field increments. Further analyses showed that the magnetic discontinuities are not distributed without correlations, but rather that non-Poisson correlations, possibly in the form of burstiness or voids, are present in the data at least up to the typical correlation scale. The discontinuities or bursty coherent structures represent in this view the current sheets that form between magnetic flux tubes which may be a signature of intermittent, anisotropic, fully developed MHD turbulence. © 2010 Elsevier Ltd. All rights reserved. All rights reserved.
publishDate 2010
dc.date.none.fl_str_mv 2010-12
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/11336/57201
Greco, Andres Francisco; Servidio, S.; Matthaeus, W.H.; Dmitruk, Pablo Ariel; Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind; Pergamon-Elsevier Science Ltd; Planetary and Space Science; 58; 14-15; 12-2010; 1895-1899
0032-0633
CONICET Digital
CONICET
url http://hdl.handle.net/11336/57201
identifier_str_mv Greco, Andres Francisco; Servidio, S.; Matthaeus, W.H.; Dmitruk, Pablo Ariel; Intermittent structures and magnetic discontinuities on small scales in MHD simulations and solar wind; Pergamon-Elsevier Science Ltd; Planetary and Space Science; 58; 14-15; 12-2010; 1895-1899
0032-0633
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/j.pss.2010.08.019
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 Pergamon-Elsevier Science Ltd
publisher.none.fl_str_mv Pergamon-Elsevier Science Ltd
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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score 13.22299

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