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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/78174
Ver los metadatos del registro completo
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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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1842269878048784384 |
score |
13.11938 |