Emergence of intermittent structures and reconnection in MHD turbulence
- Autores
- Greco, Antonella; Servidio, Sergio; Matthaeus, William H.; Dmitruk, Pablo Ariel
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union.
Fil: Greco, Antonella. Università della Calabria; Italia
Fil: Servidio, Sergio. Università della Calabria; Italia
Fil: Matthaeus, William H.. University of Delaware; Estados Unidos
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
-
(Magnetohydrodynamics:) Mhd
(Sun:) Solar Wind
Methods: Numerical
Turbulence - 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:11336/56970
Ver los metadatos del registro completo
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Emergence of intermittent structures and reconnection in MHD turbulenceGreco, AntonellaServidio, SergioMatthaeus, William H.Dmitruk, Pablo Ariel(Magnetohydrodynamics:) Mhd(Sun:) Solar WindMethods: NumericalTurbulencehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union.Fil: Greco, Antonella. Università della Calabria; ItaliaFil: Servidio, Sergio. Università della Calabria; ItaliaFil: Matthaeus, William H.. University of Delaware; Estados UnidosFil: 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; ArgentinaCUP2010-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/56970Greco, Antonella; Servidio, Sergio; Matthaeus, William H.; Dmitruk, Pablo Ariel; Emergence of intermittent structures and reconnection in MHD turbulence; CUP; Proceedings of the International Astronomical Union; 6; S274; 9-2010; 116-1191743-9221CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1017/S1743921311006697info:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/emergence-of-intermittent-structures-and-reconnection-in-mhd-turbulence/72B67811A4836F919B1F095AAF80DCB7info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:43:26Zoai:ri.conicet.gov.ar:11336/56970instacron: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 10:43:27.271CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Emergence of intermittent structures and reconnection in MHD turbulence |
title |
Emergence of intermittent structures and reconnection in MHD turbulence |
spellingShingle |
Emergence of intermittent structures and reconnection in MHD turbulence Greco, Antonella (Magnetohydrodynamics:) Mhd (Sun:) Solar Wind Methods: Numerical Turbulence |
title_short |
Emergence of intermittent structures and reconnection in MHD turbulence |
title_full |
Emergence of intermittent structures and reconnection in MHD turbulence |
title_fullStr |
Emergence of intermittent structures and reconnection in MHD turbulence |
title_full_unstemmed |
Emergence of intermittent structures and reconnection in MHD turbulence |
title_sort |
Emergence of intermittent structures and reconnection in MHD turbulence |
dc.creator.none.fl_str_mv |
Greco, Antonella Servidio, Sergio Matthaeus, William H. Dmitruk, Pablo Ariel |
author |
Greco, Antonella |
author_facet |
Greco, Antonella Servidio, Sergio Matthaeus, William H. Dmitruk, Pablo Ariel |
author_role |
author |
author2 |
Servidio, Sergio Matthaeus, William H. Dmitruk, Pablo Ariel |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
(Magnetohydrodynamics:) Mhd (Sun:) Solar Wind Methods: Numerical Turbulence |
topic |
(Magnetohydrodynamics:) Mhd (Sun:) Solar Wind Methods: Numerical 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 |
In recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union. Fil: Greco, Antonella. Università della Calabria; Italia Fil: Servidio, Sergio. Università della Calabria; Italia Fil: Matthaeus, William H.. University of Delaware; Estados Unidos 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 recent analyses of numerical simulation and solar wind dataset, the idea that the magnetic discontinuities may be related to intermittent structures that appear spontaneously in MHD turbulence has been explored in details. These studies are consistent with the hypothesis that discontinuity events founds in the solar wind might be of local origin as well, i.e. a by-product of the turbulent evolution of magnetic fluctuations. Using simulations of 2D MHD turbulence, we are exploring a possible link between tangential discontinuities and magnetic reconnection. The goal is to develop numerical algorithms that may be useful for solar wind applications. © 2011 International Astronomical Union. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-09 |
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/11336/56970 Greco, Antonella; Servidio, Sergio; Matthaeus, William H.; Dmitruk, Pablo Ariel; Emergence of intermittent structures and reconnection in MHD turbulence; CUP; Proceedings of the International Astronomical Union; 6; S274; 9-2010; 116-119 1743-9221 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/56970 |
identifier_str_mv |
Greco, Antonella; Servidio, Sergio; Matthaeus, William H.; Dmitruk, Pablo Ariel; Emergence of intermittent structures and reconnection in MHD turbulence; CUP; Proceedings of the International Astronomical Union; 6; S274; 9-2010; 116-119 1743-9221 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1017/S1743921311006697 info:eu-repo/semantics/altIdentifier/url/https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/emergence-of-intermittent-structures-and-reconnection-in-mhd-turbulence/72B67811A4836F919B1F095AAF80DCB7 |
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 |
CUP |
publisher.none.fl_str_mv |
CUP |
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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1844614469719687168 |
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13.070432 |