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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/79226
Ver los metadatos del registro completo
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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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1844614407109214208 |
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13.070432 |