A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001

Autores
Farrugia, C. J.; Gratton, Fausto Tulio Livio; Gnavi, G.; Torbert, R.; Wilson, L. B.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present an example of a boundary layer tailward of the dawn terminator which is entirely populated by rolled-up flow vortices. Observations were made by Wind on October 24, 2001 as the spacecraft moved across the region at X -13 RE. Interplanetary conditions were steady with a near-radial IMF. Approximately 15 vortices were observed over the 1.5 hr duration of Wind?s crossing, each lasting 5 min. The rolling-up is inferred from the presence of a hot tenuous plasma being accelerated to speeds higherthan in the adjoining magnetosheath, a circumstance which has been shown to be a reliable signature of this in single-spacecraft observations [Takagi et al., 2006]. A blob of cold dense plasma 12 was entrained in each vortex, at whose leading edge abrupt polarity changes of field and velocity components at current sheets were regularly observed. In the frame of the average boundary layer velocity, the dense blobs were moving predominantly sunward and their scale size along X was 8.4 RE. Inquiring into the generation mechanism of the vortices, we analyze the stability of the boundary layer to sheared flows using compressible magnetohydrodynamic Kelvin?Helmholtz theory with continuous profiles for the physical quantities. We input parameters from (i) the exact theory of magnetosheath flow under aligned solar wind field and flow vectors [Spreiter and Rizzi, 1974] near the terminator, and (ii) the Wind data. It is shown that the configuration is indeed KH unstable. This is the first reported example of KH-unstable waves at the magnetopause under a radial IMF.
Fil: Farrugia, C. J.. University Of New Hampshire; 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: Gnavi, G.. 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: Torbert, R.. University Of New Hampshire; Estados Unidos
Fil: Wilson, L. B.. University Of New Hampshire; Estados Unidos
Materia
K-H VORTICES
NEAR-RADIAL IMF
VORTICAL BOUNDARY LAYER
MAGNETOTAIL BOUNDARY LAYERS
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:11336/79226

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spelling A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001Farrugia, C. J.Gratton, Fausto Tulio LivioGnavi, G.Torbert, R.Wilson, L. B.K-H VORTICESNEAR-RADIAL IMFVORTICAL BOUNDARY LAYERMAGNETOTAIL BOUNDARY LAYERShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present an example of a boundary layer tailward of the dawn terminator which is entirely populated by rolled-up flow vortices. Observations were made by Wind on October 24, 2001 as the spacecraft moved across the region at X -13 RE. Interplanetary conditions were steady with a near-radial IMF. Approximately 15 vortices were observed over the 1.5 hr duration of Wind?s crossing, each lasting 5 min. The rolling-up is inferred from the presence of a hot tenuous plasma being accelerated to speeds higherthan in the adjoining magnetosheath, a circumstance which has been shown to be a reliable signature of this in single-spacecraft observations [Takagi et al., 2006]. A blob of cold dense plasma 12 was entrained in each vortex, at whose leading edge abrupt polarity changes of field and velocity components at current sheets were regularly observed. In the frame of the average boundary layer velocity, the dense blobs were moving predominantly sunward and their scale size along X was 8.4 RE. Inquiring into the generation mechanism of the vortices, we analyze the stability of the boundary layer to sheared flows using compressible magnetohydrodynamic Kelvin?Helmholtz theory with continuous profiles for the physical quantities. We input parameters from (i) the exact theory of magnetosheath flow under aligned solar wind field and flow vectors [Spreiter and Rizzi, 1974] near the terminator, and (ii) the Wind data. It is shown that the configuration is indeed KH unstable. This is the first reported example of KH-unstable waves at the magnetopause under a radial IMF.Fil: Farrugia, C. J.. University Of New Hampshire; 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: Gnavi, G.. 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: Torbert, R.. University Of New Hampshire; Estados UnidosFil: Wilson, L. B.. University Of New Hampshire; Estados UnidosAmerican Geophysical Union2014-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/79226Farrugia, C. J.; Gratton, Fausto Tulio Livio; Gnavi, G.; Torbert, R.; Wilson, L. B.; A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001; American Geophysical Union; Journal of Geophysical Research; 119; 1; 6-2014; 4572-45900148-0227CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1002/2013JA019578info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:38:26Zoai:ri.conicet.gov.ar:11336/79226instacron: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 10:38:27.213CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
title A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
spellingShingle A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
Farrugia, C. J.
K-H VORTICES
NEAR-RADIAL IMF
VORTICAL BOUNDARY LAYER
MAGNETOTAIL BOUNDARY LAYERS
title_short A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
title_full A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
title_fullStr A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
title_full_unstemmed A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
title_sort A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001
dc.creator.none.fl_str_mv Farrugia, C. J.
Gratton, Fausto Tulio Livio
Gnavi, G.
Torbert, R.
Wilson, L. B.
author Farrugia, C. J.
author_facet Farrugia, C. J.
Gratton, Fausto Tulio Livio
Gnavi, G.
Torbert, R.
Wilson, L. B.
author_role author
author2 Gratton, Fausto Tulio Livio
Gnavi, G.
Torbert, R.
Wilson, L. B.
author2_role author
author
author
author
dc.subject.none.fl_str_mv K-H VORTICES
NEAR-RADIAL IMF
VORTICAL BOUNDARY LAYER
MAGNETOTAIL BOUNDARY LAYERS
topic K-H VORTICES
NEAR-RADIAL IMF
VORTICAL BOUNDARY LAYER
MAGNETOTAIL BOUNDARY LAYERS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present an example of a boundary layer tailward of the dawn terminator which is entirely populated by rolled-up flow vortices. Observations were made by Wind on October 24, 2001 as the spacecraft moved across the region at X -13 RE. Interplanetary conditions were steady with a near-radial IMF. Approximately 15 vortices were observed over the 1.5 hr duration of Wind?s crossing, each lasting 5 min. The rolling-up is inferred from the presence of a hot tenuous plasma being accelerated to speeds higherthan in the adjoining magnetosheath, a circumstance which has been shown to be a reliable signature of this in single-spacecraft observations [Takagi et al., 2006]. A blob of cold dense plasma 12 was entrained in each vortex, at whose leading edge abrupt polarity changes of field and velocity components at current sheets were regularly observed. In the frame of the average boundary layer velocity, the dense blobs were moving predominantly sunward and their scale size along X was 8.4 RE. Inquiring into the generation mechanism of the vortices, we analyze the stability of the boundary layer to sheared flows using compressible magnetohydrodynamic Kelvin?Helmholtz theory with continuous profiles for the physical quantities. We input parameters from (i) the exact theory of magnetosheath flow under aligned solar wind field and flow vectors [Spreiter and Rizzi, 1974] near the terminator, and (ii) the Wind data. It is shown that the configuration is indeed KH unstable. This is the first reported example of KH-unstable waves at the magnetopause under a radial IMF.
Fil: Farrugia, C. J.. University Of New Hampshire; 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: Gnavi, G.. 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: Torbert, R.. University Of New Hampshire; Estados Unidos
Fil: Wilson, L. B.. University Of New Hampshire; Estados Unidos
description We present an example of a boundary layer tailward of the dawn terminator which is entirely populated by rolled-up flow vortices. Observations were made by Wind on October 24, 2001 as the spacecraft moved across the region at X -13 RE. Interplanetary conditions were steady with a near-radial IMF. Approximately 15 vortices were observed over the 1.5 hr duration of Wind?s crossing, each lasting 5 min. The rolling-up is inferred from the presence of a hot tenuous plasma being accelerated to speeds higherthan in the adjoining magnetosheath, a circumstance which has been shown to be a reliable signature of this in single-spacecraft observations [Takagi et al., 2006]. A blob of cold dense plasma 12 was entrained in each vortex, at whose leading edge abrupt polarity changes of field and velocity components at current sheets were regularly observed. In the frame of the average boundary layer velocity, the dense blobs were moving predominantly sunward and their scale size along X was 8.4 RE. Inquiring into the generation mechanism of the vortices, we analyze the stability of the boundary layer to sheared flows using compressible magnetohydrodynamic Kelvin?Helmholtz theory with continuous profiles for the physical quantities. We input parameters from (i) the exact theory of magnetosheath flow under aligned solar wind field and flow vectors [Spreiter and Rizzi, 1974] near the terminator, and (ii) the Wind data. It is shown that the configuration is indeed KH unstable. This is the first reported example of KH-unstable waves at the magnetopause under a radial IMF.
publishDate 2014
dc.date.none.fl_str_mv 2014-06
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/11336/79226
Farrugia, C. J.; Gratton, Fausto Tulio Livio; Gnavi, G.; Torbert, R.; Wilson, L. B.; A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001; American Geophysical Union; Journal of Geophysical Research; 119; 1; 6-2014; 4572-4590
0148-0227
CONICET Digital
CONICET
url http://hdl.handle.net/11336/79226
identifier_str_mv Farrugia, C. J.; Gratton, Fausto Tulio Livio; Gnavi, G.; Torbert, R.; Wilson, L. B.; A Vortical Dawn Flank Boundary Layer for Near-Radial IMF: Wind Observations on October 24, 2001; American Geophysical Union; Journal of Geophysical Research; 119; 1; 6-2014; 4572-4590
0148-0227
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1002/2013JA019578
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 Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
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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