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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/57201
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T09:36:14Zoai: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:34982025-09-29 09:36:14.664CONICET 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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13.070432 |