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dc.contributor.author
Lund, E.J.  
dc.contributor.author
Farrugia, C. J.  
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Sandholt, P. E.  
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Kistler, L. M.  
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Fairfield, D. H.  
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Gratton, Fausto Tulio Livio  
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Cowley, S. W. H.  
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Wild, J. A.  
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Mouikis, C. G.  
dc.contributor.author
Dunlop, M. W.  
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Reme, H.  
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Carlson, C. W.  
dc.date.available
2020-04-22T15:47:42Z  
dc.date.issued
2006-01  
dc.identifier.citation
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  
dc.identifier.issn
0273-1177  
dc.identifier.uri
http://hdl.handle.net/11336/103287  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Elsevier  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Boundary layers  
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Solar wind–magnetosphere coupling  
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Multispacecraft measurements  
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Reconnection  
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Kelvin–Helmholtz instability  
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Física de los Fluidos y Plasma  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
The changing topology of the duskside magnetopause boundary layer in relation to IMF orientation  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2020-04-21T15:25:46Z  
dc.journal.volume
37  
dc.journal.number
3  
dc.journal.pagination
497-500  
dc.journal.pais
Países Bajos  
dc.journal.ciudad
Amsterdam  
dc.description.fil
Fil: Lund, E.J.. University of New Hampshire; Estados Unidos  
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Fil: Farrugia, C. J.. University of New Hampshire; Estados Unidos  
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Fil: Sandholt, P. E.. University of Oslo; Noruega  
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Fil: Kistler, L. M.. University of New Hampshire; Estados Unidos  
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Fil: Fairfield, D. H.. Goddard Space Flight Center; Estados Unidos  
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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  
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Fil: Cowley, S. W. H.. University of Leicester; Reino Unido  
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Fil: Wild, J. A.. University of Leicester; Reino Unido  
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Fil: Mouikis, C. G.. Goddard Space Flight Center; Estados Unidos  
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Fil: Dunlop, M. W.. Rutherford Appleton Laboratory; Reino Unido  
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Fil: Reme, H.. Centre d'Etude Spatiale des Rayonnements; Francia  
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Fil: Carlson, C. W.. University of California; Estados Unidos  
dc.journal.title
Advances in Space Research  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0273117704008841  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.asr.2004.11.035