The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation
- Autores
- Lund, E.J.; Farrugia, C. J.; Sandholt, P. E.; Kistler, L. M.; Fairfield, D. H.; Gratton, Fausto Tulio Livio; Cowley, S. W. H.; Wild, J. A.; Mouikis, C. G.; Dunlop, M. W.; Reme, H.; Carlson, C. W.
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- On 7 December 2000, Cluster made an extended outbound radial traversal of the duskside magnetopause boundary layer. The long duration of the crossing, during which Cluster spent several hours within 2RE of the nominal magnetopause, allows us to deconvolve the structure of this boundary layer in its dependence on interplanetary parameters. We present evidence that as the interplanetary magnetic field (IMF) changed in discontinuous jumps from southward to northward, the magnetic topology of the boundary layer evolved from open to closed. Reconnection signatures, including enhanced flows observed locally at Cluster and ion energy dispersion signatures observed by FAST near Cluster’s magnetic footpoint, appeared while the IMF was southward. When the IMF turned nearly due northward, Cluster observed 75-s (Pc 4) oscillations which we attribute to the Kelvin-Helmholtz instability.
Fil: Lund, E.J.. University of New Hampshire; Estados Unidos
Fil: Farrugia, C. J.. University of New Hampshire; Estados Unidos
Fil: Sandholt, P. E.. University of Oslo; Noruega
Fil: Kistler, L. M.. University of New Hampshire; Estados Unidos
Fil: Fairfield, D. H.. Goddard Space Flight Center; Estados Unidos
Fil: Gratton, Fausto Tulio Livio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; Argentina
Fil: Cowley, S. W. H.. University of Leicester; Reino Unido
Fil: Wild, J. A.. University of Leicester; Reino Unido
Fil: Mouikis, C. G.. Goddard Space Flight Center; Estados Unidos
Fil: Dunlop, M. W.. Rutherford Appleton Laboratory; Reino Unido
Fil: Reme, H.. Centre d'Etude Spatiale des Rayonnements; Francia
Fil: Carlson, C. W.. University of California; Estados Unidos - Materia
-
Boundary layers
Solar wind–magnetosphere coupling
Multispacecraft measurements
Reconnection
Kelvin–Helmholtz instability - 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:11336/103287
Ver los metadatos del registro completo
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The changing topology of the duskside magnetopause boundary layer in relation to IMF orientationLund, E.J.Farrugia, C. J.Sandholt, P. E.Kistler, L. M.Fairfield, D. H.Gratton, Fausto Tulio LivioCowley, S. W. H.Wild, J. A.Mouikis, C. G.Dunlop, M. W.Reme, H.Carlson, C. W.Boundary layersSolar wind–magnetosphere couplingMultispacecraft measurementsReconnectionKelvin–Helmholtz instabilityhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1On 7 December 2000, Cluster made an extended outbound radial traversal of the duskside magnetopause boundary layer. The long duration of the crossing, during which Cluster spent several hours within 2RE of the nominal magnetopause, allows us to deconvolve the structure of this boundary layer in its dependence on interplanetary parameters. We present evidence that as the interplanetary magnetic field (IMF) changed in discontinuous jumps from southward to northward, the magnetic topology of the boundary layer evolved from open to closed. Reconnection signatures, including enhanced flows observed locally at Cluster and ion energy dispersion signatures observed by FAST near Cluster’s magnetic footpoint, appeared while the IMF was southward. When the IMF turned nearly due northward, Cluster observed 75-s (Pc 4) oscillations which we attribute to the Kelvin-Helmholtz instability.Fil: Lund, E.J.. University of New Hampshire; Estados UnidosFil: Farrugia, C. J.. University of New Hampshire; Estados UnidosFil: Sandholt, P. E.. University of Oslo; NoruegaFil: Kistler, L. M.. University of New Hampshire; Estados UnidosFil: Fairfield, D. H.. Goddard Space Flight Center; Estados UnidosFil: Gratton, Fausto Tulio Livio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; ArgentinaFil: Cowley, S. W. H.. University of Leicester; Reino UnidoFil: Wild, J. A.. University of Leicester; Reino UnidoFil: Mouikis, C. G.. Goddard Space Flight Center; Estados UnidosFil: Dunlop, M. W.. Rutherford Appleton Laboratory; Reino UnidoFil: Reme, H.. Centre d'Etude Spatiale des Rayonnements; FranciaFil: Carlson, C. W.. University of California; Estados UnidosElsevier2006-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/103287Lund, E.J.; Farrugia, C. J.; Sandholt, P. E.; Kistler, L. M.; Fairfield, D. H.; et al.; The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation; Elsevier; Advances in Space Research; 37; 3; 1-2006; 497-5000273-1177CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0273117704008841info:eu-repo/semantics/altIdentifier/doi/10.1016/j.asr.2004.11.035info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:59:27Zoai:ri.conicet.gov.ar:11336/103287instacron: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 09:59:27.317CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
title |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
spellingShingle |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation Lund, E.J. Boundary layers Solar wind–magnetosphere coupling Multispacecraft measurements Reconnection Kelvin–Helmholtz instability |
title_short |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
title_full |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
title_fullStr |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
title_full_unstemmed |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
title_sort |
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation |
dc.creator.none.fl_str_mv |
Lund, E.J. Farrugia, C. J. Sandholt, P. E. Kistler, L. M. Fairfield, D. H. Gratton, Fausto Tulio Livio Cowley, S. W. H. Wild, J. A. Mouikis, C. G. Dunlop, M. W. Reme, H. Carlson, C. W. |
author |
Lund, E.J. |
author_facet |
Lund, E.J. Farrugia, C. J. Sandholt, P. E. Kistler, L. M. Fairfield, D. H. Gratton, Fausto Tulio Livio Cowley, S. W. H. Wild, J. A. Mouikis, C. G. Dunlop, M. W. Reme, H. Carlson, C. W. |
author_role |
author |
author2 |
Farrugia, C. J. Sandholt, P. E. Kistler, L. M. Fairfield, D. H. Gratton, Fausto Tulio Livio Cowley, S. W. H. Wild, J. A. Mouikis, C. G. Dunlop, M. W. Reme, H. Carlson, C. W. |
author2_role |
author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Boundary layers Solar wind–magnetosphere coupling Multispacecraft measurements Reconnection Kelvin–Helmholtz instability |
topic |
Boundary layers Solar wind–magnetosphere coupling Multispacecraft measurements Reconnection Kelvin–Helmholtz instability |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
On 7 December 2000, Cluster made an extended outbound radial traversal of the duskside magnetopause boundary layer. The long duration of the crossing, during which Cluster spent several hours within 2RE of the nominal magnetopause, allows us to deconvolve the structure of this boundary layer in its dependence on interplanetary parameters. We present evidence that as the interplanetary magnetic field (IMF) changed in discontinuous jumps from southward to northward, the magnetic topology of the boundary layer evolved from open to closed. Reconnection signatures, including enhanced flows observed locally at Cluster and ion energy dispersion signatures observed by FAST near Cluster’s magnetic footpoint, appeared while the IMF was southward. When the IMF turned nearly due northward, Cluster observed 75-s (Pc 4) oscillations which we attribute to the Kelvin-Helmholtz instability. Fil: Lund, E.J.. University of New Hampshire; Estados Unidos Fil: Farrugia, C. J.. University of New Hampshire; Estados Unidos Fil: Sandholt, P. E.. University of Oslo; Noruega Fil: Kistler, L. M.. University of New Hampshire; Estados Unidos Fil: Fairfield, D. H.. Goddard Space Flight Center; Estados Unidos Fil: Gratton, Fausto Tulio Livio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física del Plasma. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física del Plasma; Argentina Fil: Cowley, S. W. H.. University of Leicester; Reino Unido Fil: Wild, J. A.. University of Leicester; Reino Unido Fil: Mouikis, C. G.. Goddard Space Flight Center; Estados Unidos Fil: Dunlop, M. W.. Rutherford Appleton Laboratory; Reino Unido Fil: Reme, H.. Centre d'Etude Spatiale des Rayonnements; Francia Fil: Carlson, C. W.. University of California; Estados Unidos |
description |
On 7 December 2000, Cluster made an extended outbound radial traversal of the duskside magnetopause boundary layer. The long duration of the crossing, during which Cluster spent several hours within 2RE of the nominal magnetopause, allows us to deconvolve the structure of this boundary layer in its dependence on interplanetary parameters. We present evidence that as the interplanetary magnetic field (IMF) changed in discontinuous jumps from southward to northward, the magnetic topology of the boundary layer evolved from open to closed. Reconnection signatures, including enhanced flows observed locally at Cluster and ion energy dispersion signatures observed by FAST near Cluster’s magnetic footpoint, appeared while the IMF was southward. When the IMF turned nearly due northward, Cluster observed 75-s (Pc 4) oscillations which we attribute to the Kelvin-Helmholtz instability. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-01 |
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/11336/103287 Lund, E.J.; Farrugia, C. J.; Sandholt, P. E.; Kistler, L. M.; Fairfield, D. H.; et al.; The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation; Elsevier; Advances in Space Research; 37; 3; 1-2006; 497-500 0273-1177 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/103287 |
identifier_str_mv |
Lund, E.J.; Farrugia, C. J.; Sandholt, P. E.; Kistler, L. M.; Fairfield, D. H.; et al.; The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation; Elsevier; Advances in Space Research; 37; 3; 1-2006; 497-500 0273-1177 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0273117704008841 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.asr.2004.11.035 |
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 |
Elsevier |
publisher.none.fl_str_mv |
Elsevier |
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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1844613763819372544 |
score |
13.070432 |