Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres

Autores
Valladares, Cesar Enrique; Villalobos, J.; Hei, M. A.; Sheehan, R; Basu, Su; Mackenzie, E.; Doherty, P. H.; Rios, Victor Hugo
Año de publicación
2009
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Measurements of total electron content (TEC) using 263 GPS receivers located in the North and South America continents are presented to demonstrate the simultaneous existence of traveling ionospheric disturbances (TID) at high, mid, and low latitudes, and in both Northern and Southern Hemispheres. The TID observations pertain to the magnetically disturbed period of 29–30 October 2003 also known as the Halloween storm. The excellent quality of the TEC measurements makes it possible to calculate and remove the diurnal variability of TEC and then estimate the amplitude, wavelength, spectral characteristics of the perturbations, and the approximate velocity of the AGW. On 29 October 2003 between 17:00 and 19:00 UT, there existed a sequence of TEC perturbations (TECP), which were associated with the transit of atmospheric gravity waves (AGW) propagating from both auroral regions toward the geographic equator. A marked difference was found between the northern and southern perturbations. In the Northern Hemisphere, the preferred horizontal wavelength varies between 1500 and 1800 km; the propagation velocity is near 700 m/s and the perturbation amplitude about 1 TEC unit (TECu). South of the geographic equator the wavelength of the TECP is as large as 2700 km, the velocity is about 550 m/s, and the TECP amplitude is 3 TECu. Concurrently with our observations, the Jicamarca digisonde observed virtual height traces that exhibited typical features that are associated with TIDs. Here, it is suggested that differences in the local conductivity between northern and southern auroral ovals create a different Joule heating energy term. The quality of these observations illustrates the merits of GPS receivers to probe the ionosphere and thermosphere
Fil: Valladares, Cesar Enrique. Boston College; Estados Unidos
Fil: Villalobos, J.. Universidad Nacional de Colombia; Colombia
Fil: Hei, M. A.. Boston College; Estados Unidos
Fil: Sheehan, R. Boston College; Estados Unidos
Fil: Basu, Su. Boston University; Estados Unidos
Fil: Mackenzie, E.. Boston College; Estados Unidos
Fil: Doherty, P. H.. Boston College; Estados Unidos
Fil: Rios, Victor Hugo. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina
Materia
Ionospheric
Disturbances
Hemispheres
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:11336/78174

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network_name_str CONICET Digital (CONICET)
spelling Simultaneuos observation of traveling ionospheric disturbances in the northern HemispheresValladares, Cesar EnriqueVillalobos, J.Hei, M. A.Sheehan, RBasu, SuMackenzie, E.Doherty, P. H.Rios, Victor HugoIonosphericDisturbancesHemisphereshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Measurements of total electron content (TEC) using 263 GPS receivers located in the North and South America continents are presented to demonstrate the simultaneous existence of traveling ionospheric disturbances (TID) at high, mid, and low latitudes, and in both Northern and Southern Hemispheres. The TID observations pertain to the magnetically disturbed period of 29–30 October 2003 also known as the Halloween storm. The excellent quality of the TEC measurements makes it possible to calculate and remove the diurnal variability of TEC and then estimate the amplitude, wavelength, spectral characteristics of the perturbations, and the approximate velocity of the AGW. On 29 October 2003 between 17:00 and 19:00 UT, there existed a sequence of TEC perturbations (TECP), which were associated with the transit of atmospheric gravity waves (AGW) propagating from both auroral regions toward the geographic equator. A marked difference was found between the northern and southern perturbations. In the Northern Hemisphere, the preferred horizontal wavelength varies between 1500 and 1800 km; the propagation velocity is near 700 m/s and the perturbation amplitude about 1 TEC unit (TECu). South of the geographic equator the wavelength of the TECP is as large as 2700 km, the velocity is about 550 m/s, and the TECP amplitude is 3 TECu. Concurrently with our observations, the Jicamarca digisonde observed virtual height traces that exhibited typical features that are associated with TIDs. Here, it is suggested that differences in the local conductivity between northern and southern auroral ovals create a different Joule heating energy term. The quality of these observations illustrates the merits of GPS receivers to probe the ionosphere and thermosphereFil: Valladares, Cesar Enrique. Boston College; Estados UnidosFil: Villalobos, J.. Universidad Nacional de Colombia; ColombiaFil: Hei, M. A.. Boston College; Estados UnidosFil: Sheehan, R. Boston College; Estados UnidosFil: Basu, Su. Boston University; Estados UnidosFil: Mackenzie, E.. Boston College; Estados UnidosFil: Doherty, P. H.. Boston College; Estados UnidosFil: Rios, Victor Hugo. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; ArgentinaCopernicus Publications2009-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/78174Valladares, Cesar Enrique; Villalobos, J.; Hei, M. A.; Sheehan, R; Basu, Su; et al.; Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres; Copernicus Publications; Annales Geophysicae; 27; 4; 6-2009; 1-80992-76891432-0576CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.5194/angeo-27-1501-2009info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T10:04:49Zoai:ri.conicet.gov.ar:11336/78174instacron: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:34982025-09-03 10:04:49.584CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
title Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
spellingShingle Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
Valladares, Cesar Enrique
Ionospheric
Disturbances
Hemispheres
title_short Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
title_full Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
title_fullStr Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
title_full_unstemmed Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
title_sort Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres
dc.creator.none.fl_str_mv Valladares, Cesar Enrique
Villalobos, J.
Hei, M. A.
Sheehan, R
Basu, Su
Mackenzie, E.
Doherty, P. H.
Rios, Victor Hugo
author Valladares, Cesar Enrique
author_facet Valladares, Cesar Enrique
Villalobos, J.
Hei, M. A.
Sheehan, R
Basu, Su
Mackenzie, E.
Doherty, P. H.
Rios, Victor Hugo
author_role author
author2 Villalobos, J.
Hei, M. A.
Sheehan, R
Basu, Su
Mackenzie, E.
Doherty, P. H.
Rios, Victor Hugo
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Ionospheric
Disturbances
Hemispheres
topic Ionospheric
Disturbances
Hemispheres
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Measurements of total electron content (TEC) using 263 GPS receivers located in the North and South America continents are presented to demonstrate the simultaneous existence of traveling ionospheric disturbances (TID) at high, mid, and low latitudes, and in both Northern and Southern Hemispheres. The TID observations pertain to the magnetically disturbed period of 29–30 October 2003 also known as the Halloween storm. The excellent quality of the TEC measurements makes it possible to calculate and remove the diurnal variability of TEC and then estimate the amplitude, wavelength, spectral characteristics of the perturbations, and the approximate velocity of the AGW. On 29 October 2003 between 17:00 and 19:00 UT, there existed a sequence of TEC perturbations (TECP), which were associated with the transit of atmospheric gravity waves (AGW) propagating from both auroral regions toward the geographic equator. A marked difference was found between the northern and southern perturbations. In the Northern Hemisphere, the preferred horizontal wavelength varies between 1500 and 1800 km; the propagation velocity is near 700 m/s and the perturbation amplitude about 1 TEC unit (TECu). South of the geographic equator the wavelength of the TECP is as large as 2700 km, the velocity is about 550 m/s, and the TECP amplitude is 3 TECu. Concurrently with our observations, the Jicamarca digisonde observed virtual height traces that exhibited typical features that are associated with TIDs. Here, it is suggested that differences in the local conductivity between northern and southern auroral ovals create a different Joule heating energy term. The quality of these observations illustrates the merits of GPS receivers to probe the ionosphere and thermosphere
Fil: Valladares, Cesar Enrique. Boston College; Estados Unidos
Fil: Villalobos, J.. Universidad Nacional de Colombia; Colombia
Fil: Hei, M. A.. Boston College; Estados Unidos
Fil: Sheehan, R. Boston College; Estados Unidos
Fil: Basu, Su. Boston University; Estados Unidos
Fil: Mackenzie, E.. Boston College; Estados Unidos
Fil: Doherty, P. H.. Boston College; Estados Unidos
Fil: Rios, Victor Hugo. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina
description Measurements of total electron content (TEC) using 263 GPS receivers located in the North and South America continents are presented to demonstrate the simultaneous existence of traveling ionospheric disturbances (TID) at high, mid, and low latitudes, and in both Northern and Southern Hemispheres. The TID observations pertain to the magnetically disturbed period of 29–30 October 2003 also known as the Halloween storm. The excellent quality of the TEC measurements makes it possible to calculate and remove the diurnal variability of TEC and then estimate the amplitude, wavelength, spectral characteristics of the perturbations, and the approximate velocity of the AGW. On 29 October 2003 between 17:00 and 19:00 UT, there existed a sequence of TEC perturbations (TECP), which were associated with the transit of atmospheric gravity waves (AGW) propagating from both auroral regions toward the geographic equator. A marked difference was found between the northern and southern perturbations. In the Northern Hemisphere, the preferred horizontal wavelength varies between 1500 and 1800 km; the propagation velocity is near 700 m/s and the perturbation amplitude about 1 TEC unit (TECu). South of the geographic equator the wavelength of the TECP is as large as 2700 km, the velocity is about 550 m/s, and the TECP amplitude is 3 TECu. Concurrently with our observations, the Jicamarca digisonde observed virtual height traces that exhibited typical features that are associated with TIDs. Here, it is suggested that differences in the local conductivity between northern and southern auroral ovals create a different Joule heating energy term. The quality of these observations illustrates the merits of GPS receivers to probe the ionosphere and thermosphere
publishDate 2009
dc.date.none.fl_str_mv 2009-06
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/11336/78174
Valladares, Cesar Enrique; Villalobos, J.; Hei, M. A.; Sheehan, R; Basu, Su; et al.; Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres; Copernicus Publications; Annales Geophysicae; 27; 4; 6-2009; 1-8
0992-7689
1432-0576
CONICET Digital
CONICET
url http://hdl.handle.net/11336/78174
identifier_str_mv Valladares, Cesar Enrique; Villalobos, J.; Hei, M. A.; Sheehan, R; Basu, Su; et al.; Simultaneuos observation of traveling ionospheric disturbances in the northern Hemispheres; Copernicus Publications; Annales Geophysicae; 27; 4; 6-2009; 1-8
0992-7689
1432-0576
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.5194/angeo-27-1501-2009
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 Copernicus Publications
publisher.none.fl_str_mv Copernicus Publications
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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