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dc.contributor.author
Lund, E.J.
dc.contributor.author
Farrugia, C. J.
dc.contributor.author
Sandholt, P. E.
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Kistler, L. M.
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Fairfield, D. H.
dc.contributor.author
Gratton, Fausto Tulio Livio
dc.contributor.author
Cowley, S. W. H.
dc.contributor.author
Wild, J. A.
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Mouikis, C. G.
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Dunlop, M. W.
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Reme, H.
dc.contributor.author
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
dc.description.fil
Fil: Sandholt, P. E.. University of Oslo; Noruega
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Fil: Kistler, L. M.. University of New Hampshire; Estados Unidos
dc.description.fil
Fil: Fairfield, D. H.. Goddard Space Flight Center; Estados Unidos
dc.description.fil
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
dc.description.fil
Fil: Cowley, S. W. H.. University of Leicester; Reino Unido
dc.description.fil
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
dc.description.fil
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
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