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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/21327
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:37:03Zoai: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:34982025-09-29 10:37:03.891CONICET 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 |
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CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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1844614391004135424 |
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13.070432 |