Spatial correlation of solar-wind turbulence from two-point measurements

Autores
Matthaeus, W. H.; Dasso, Sergio Ricardo; Weygand, J. M.; Milano, L. J.; Smith, C. W.; Kivelson, M. G.
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth’s orbit.
Fil: Matthaeus, W. H.. University of Delaware; Estados Unidos
Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Weygand, J. M.. University of California at Los Angeles; Estados Unidos
Fil: Milano, L. J.. University of Delaware; Estados Unidos
Fil: Smith, C. W.. University of New Hampshire; Estados Unidos
Fil: Kivelson, M. G.. University of California at Los Angeles; Estados Unidos
Materia
Solar Wind
Mhd
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:11336/21327
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Spatial correlation of solar-wind turbulence from two-point measurementsMatthaeus, W. H.Dasso, Sergio RicardoWeygand, J. M.Milano, L. J.Smith, C. W.Kivelson, M. G.Solar WindMhdTurbulencehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth’s orbit.Fil: Matthaeus, W. H.. University of Delaware; Estados UnidosFil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Weygand, J. M.. University of California at Los Angeles; Estados UnidosFil: Milano, L. J.. University of Delaware; Estados UnidosFil: Smith, C. W.. University of New Hampshire; Estados UnidosFil: Kivelson, M. G.. University of California at Los Angeles; Estados UnidosAmerican Physical Society2005-12-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21327Matthaeus, W. H.; Dasso, Sergio Ricardo; Weygand, J. M.; Milano, L. J.; Smith, C. W.; et al.; Spatial correlation of solar-wind turbulence from two-point measurements; American Physical Society; Physical Review Letters; 95; 23; 2-12-2005; 1-4; 2311010031-9007CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevLett.95.231101info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.95.231101info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:34:31Zoai:ri.conicet.gov.ar:11336/21327instacron: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 15:34:31.474CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Spatial correlation of solar-wind turbulence from two-point measurements
title Spatial correlation of solar-wind turbulence from two-point measurements
spellingShingle Spatial correlation of solar-wind turbulence from two-point measurements
Matthaeus, W. H.
Solar Wind
Mhd
Turbulence
title_short Spatial correlation of solar-wind turbulence from two-point measurements
title_full Spatial correlation of solar-wind turbulence from two-point measurements
title_fullStr Spatial correlation of solar-wind turbulence from two-point measurements
title_full_unstemmed Spatial correlation of solar-wind turbulence from two-point measurements
title_sort Spatial correlation of solar-wind turbulence from two-point measurements
dc.creator.none.fl_str_mv Matthaeus, W. H.
Dasso, Sergio Ricardo
Weygand, J. M.
Milano, L. J.
Smith, C. W.
Kivelson, M. G.
author Matthaeus, W. H.
author_facet Matthaeus, W. H.
Dasso, Sergio Ricardo
Weygand, J. M.
Milano, L. J.
Smith, C. W.
Kivelson, M. G.
author_role author
author2 Dasso, Sergio Ricardo
Weygand, J. M.
Milano, L. J.
Smith, C. W.
Kivelson, M. G.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Solar Wind
Mhd
Turbulence
topic Solar Wind
Mhd
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 Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth’s orbit.
Fil: Matthaeus, W. H.. University of Delaware; Estados Unidos
Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Weygand, J. M.. University of California at Los Angeles; Estados Unidos
Fil: Milano, L. J.. University of Delaware; Estados Unidos
Fil: Smith, C. W.. University of New Hampshire; Estados Unidos
Fil: Kivelson, M. G.. University of California at Los Angeles; Estados Unidos
description Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only directly quantified instance of astrophysical turbulence. Here, magnetic field correlation analysis, using for the first time only proper two-point, single time measurements, provides a key step in unraveling the space-time structure of interplanetary turbulence. Simultaneous magnetic field data from the Wind, ACE, and Cluster spacecraft are analyzed to determine the correlation (outer) scale, and the Taylor microscale near Earth’s orbit.
publishDate 2005
dc.date.none.fl_str_mv 2005-12-02
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/11336/21327
Matthaeus, W. H.; Dasso, Sergio Ricardo; Weygand, J. M.; Milano, L. J.; Smith, C. W.; et al.; Spatial correlation of solar-wind turbulence from two-point measurements; American Physical Society; Physical Review Letters; 95; 23; 2-12-2005; 1-4; 231101
0031-9007
CONICET Digital
CONICET
url http://hdl.handle.net/11336/21327
identifier_str_mv Matthaeus, W. H.; Dasso, Sergio Ricardo; Weygand, J. M.; Milano, L. J.; Smith, C. W.; et al.; Spatial correlation of solar-wind turbulence from two-point measurements; American Physical Society; Physical Review Letters; 95; 23; 2-12-2005; 1-4; 231101
0031-9007
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/PhysRevLett.95.231101
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.95.231101
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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score 13.22299

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