Intermittent MHD structures and classical discontinuities

Autores
Greco, Andres Francisco; Chuychai, P.; Matthaeus, W.H.; Servidio, S.; Dmitruk, Pablo Ariel
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We examine statistics of rapid spatial variations of the magnetic field in simulations of magnetohydrodynamic (MHD) turbulence, by analyzing intermittency properties. and by using classical methods for identifying discontinuities. The methods identify similar structures, and give very similar event distribution functions. When the results are scaled to the correlation length, the average waiting times agree with typically reported waiting times between solar wind discontinuities. Thus discontinuities may be related to flux tube boundaries and intermittent structures that appear spontaneously in MHD turbulence. Copyright 2008 by the American Geophysical Union.
Fil: Greco, Andres Francisco. Universita Della Calabria; España
Fil: Chuychai, P.. Bartol Research Institute; Estados Unidos
Fil: Matthaeus, W.H.. Bartol Research Institute; Estados Unidos
Fil: Servidio, S.. Bartol Research Institute; Estados Unidos
Fil: Dmitruk, Pablo Ariel. 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
Materia
magnetohydrodynamic
turbulence
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:11336/62198
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/62198
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Intermittent MHD structures and classical discontinuitiesGreco, Andres FranciscoChuychai, P.Matthaeus, W.H.Servidio, S.Dmitruk, Pablo Arielmagnetohydrodynamicturbulencehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We examine statistics of rapid spatial variations of the magnetic field in simulations of magnetohydrodynamic (MHD) turbulence, by analyzing intermittency properties. and by using classical methods for identifying discontinuities. The methods identify similar structures, and give very similar event distribution functions. When the results are scaled to the correlation length, the average waiting times agree with typically reported waiting times between solar wind discontinuities. Thus discontinuities may be related to flux tube boundaries and intermittent structures that appear spontaneously in MHD turbulence. Copyright 2008 by the American Geophysical Union.Fil: Greco, Andres Francisco. Universita Della Calabria; EspañaFil: Chuychai, P.. Bartol Research Institute; Estados UnidosFil: Matthaeus, W.H.. Bartol Research Institute; Estados UnidosFil: Servidio, S.. Bartol Research Institute; Estados UnidosFil: Dmitruk, Pablo Ariel. 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; ArgentinaAmerican Geophysical Union2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/62198Greco, Andres Francisco; Chuychai, P.; Matthaeus, W.H.; Servidio, S.; Dmitruk, Pablo Ariel; Intermittent MHD structures and classical discontinuities; American Geophysical Union; Geophysical Research Letters; 35; 19; 12-2008; 191111-1911140094-8276CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1029/2008GL035454info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:10:57Zoai:ri.conicet.gov.ar:11336/62198instacron: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 15:10:57.28CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Intermittent MHD structures and classical discontinuities
title Intermittent MHD structures and classical discontinuities
spellingShingle Intermittent MHD structures and classical discontinuities
Greco, Andres Francisco
magnetohydrodynamic
turbulence
title_short Intermittent MHD structures and classical discontinuities
title_full Intermittent MHD structures and classical discontinuities
title_fullStr Intermittent MHD structures and classical discontinuities
title_full_unstemmed Intermittent MHD structures and classical discontinuities
title_sort Intermittent MHD structures and classical discontinuities
dc.creator.none.fl_str_mv Greco, Andres Francisco
Chuychai, P.
Matthaeus, W.H.
Servidio, S.
Dmitruk, Pablo Ariel
author Greco, Andres Francisco
author_facet Greco, Andres Francisco
Chuychai, P.
Matthaeus, W.H.
Servidio, S.
Dmitruk, Pablo Ariel
author_role author
author2 Chuychai, P.
Matthaeus, W.H.
Servidio, S.
Dmitruk, Pablo Ariel
author2_role author
author
author
author
dc.subject.none.fl_str_mv magnetohydrodynamic
turbulence
topic magnetohydrodynamic
turbulence
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We examine statistics of rapid spatial variations of the magnetic field in simulations of magnetohydrodynamic (MHD) turbulence, by analyzing intermittency properties. and by using classical methods for identifying discontinuities. The methods identify similar structures, and give very similar event distribution functions. When the results are scaled to the correlation length, the average waiting times agree with typically reported waiting times between solar wind discontinuities. Thus discontinuities may be related to flux tube boundaries and intermittent structures that appear spontaneously in MHD turbulence. Copyright 2008 by the American Geophysical Union.
Fil: Greco, Andres Francisco. Universita Della Calabria; España
Fil: Chuychai, P.. Bartol Research Institute; Estados Unidos
Fil: Matthaeus, W.H.. Bartol Research Institute; Estados Unidos
Fil: Servidio, S.. Bartol Research Institute; Estados Unidos
Fil: Dmitruk, Pablo Ariel. 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
description We examine statistics of rapid spatial variations of the magnetic field in simulations of magnetohydrodynamic (MHD) turbulence, by analyzing intermittency properties. and by using classical methods for identifying discontinuities. The methods identify similar structures, and give very similar event distribution functions. When the results are scaled to the correlation length, the average waiting times agree with typically reported waiting times between solar wind discontinuities. Thus discontinuities may be related to flux tube boundaries and intermittent structures that appear spontaneously in MHD turbulence. Copyright 2008 by the American Geophysical Union.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
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/11336/62198
Greco, Andres Francisco; Chuychai, P.; Matthaeus, W.H.; Servidio, S.; Dmitruk, Pablo Ariel; Intermittent MHD structures and classical discontinuities; American Geophysical Union; Geophysical Research Letters; 35; 19; 12-2008; 191111-191114
0094-8276
CONICET Digital
CONICET
url http://hdl.handle.net/11336/62198
identifier_str_mv Greco, Andres Francisco; Chuychai, P.; Matthaeus, W.H.; Servidio, S.; Dmitruk, Pablo Ariel; Intermittent MHD structures and classical discontinuities; American Geophysical Union; Geophysical Research Letters; 35; 19; 12-2008; 191111-191114
0094-8276
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1029/2008GL035454
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 Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
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
_version_ 1846083257776472064
score 13.22299

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