Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011
- Autores
- Correia, Emilia; Junqueira Paz, Armanda; Gende, Mauricio Alfredo
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The vertical total electron content (VTEC) obtained from 2004 to 2011 at Comandante Ferraz Brazilian Antarctic Station (62.1°S, 58.4°W) is analyzed to study the mean diurnal, seasonal and annual variations. The maximum daytime VTEC had an annual variation that decreased from 2004 to 2008, and then starting to increase in 2009, which followed the variation of the solar activity. The daily VTEC shows good linear correlation with solar radiation intensity, which is also dependent on the solar zenithal angle. The mean diurnal VTEC shows a semiannual variation, with larger peaks in equinoxes for all years; no winter anomaly was observed, and in summer, there was no clear diurnal variation. The semiannual variation of the VTEC is also modulated by solar activity, with larger VTEC peaks when the solar activity was higher.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Geofísica
Ionosphere
Total electron content
Seasonal variation
Solar cycle - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/99989
Ver los metadatos del registro completo
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Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011Correia, EmiliaJunqueira Paz, ArmandaGende, Mauricio AlfredoGeofísicaIonosphereTotal electron contentSeasonal variationSolar cycleThe vertical total electron content (VTEC) obtained from 2004 to 2011 at Comandante Ferraz Brazilian Antarctic Station (62.1°S, 58.4°W) is analyzed to study the mean diurnal, seasonal and annual variations. The maximum daytime VTEC had an annual variation that decreased from 2004 to 2008, and then starting to increase in 2009, which followed the variation of the solar activity. The daily VTEC shows good linear correlation with solar radiation intensity, which is also dependent on the solar zenithal angle. The mean diurnal VTEC shows a semiannual variation, with larger peaks in equinoxes for all years; no winter anomaly was observed, and in summer, there was no clear diurnal variation. The semiannual variation of the VTEC is also modulated by solar activity, with larger VTEC peaks when the solar activity was higher.Facultad de Ciencias Astronómicas y Geofísicas2013-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1-5http://sedici.unlp.edu.ar/handle/10915/99989enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/23228info:eu-repo/semantics/altIdentifier/url/http://www.annalsofgeophysics.eu/index.php/annals/article/view/6223info:eu-repo/semantics/altIdentifier/issn/2037-416Xinfo:eu-repo/semantics/altIdentifier/doi/10.4401/ag-6223info:eu-repo/semantics/altIdentifier/hdl/11336/23228info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:19:56Zoai:sedici.unlp.edu.ar:10915/99989Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:19:57.135SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
title |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
spellingShingle |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 Correia, Emilia Geofísica Ionosphere Total electron content Seasonal variation Solar cycle |
title_short |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
title_full |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
title_fullStr |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
title_full_unstemmed |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
title_sort |
Characterization of GPS total electron content (GPS-TEC) in Antarctica from 2004 to 2011 |
dc.creator.none.fl_str_mv |
Correia, Emilia Junqueira Paz, Armanda Gende, Mauricio Alfredo |
author |
Correia, Emilia |
author_facet |
Correia, Emilia Junqueira Paz, Armanda Gende, Mauricio Alfredo |
author_role |
author |
author2 |
Junqueira Paz, Armanda Gende, Mauricio Alfredo |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Geofísica Ionosphere Total electron content Seasonal variation Solar cycle |
topic |
Geofísica Ionosphere Total electron content Seasonal variation Solar cycle |
dc.description.none.fl_txt_mv |
The vertical total electron content (VTEC) obtained from 2004 to 2011 at Comandante Ferraz Brazilian Antarctic Station (62.1°S, 58.4°W) is analyzed to study the mean diurnal, seasonal and annual variations. The maximum daytime VTEC had an annual variation that decreased from 2004 to 2008, and then starting to increase in 2009, which followed the variation of the solar activity. The daily VTEC shows good linear correlation with solar radiation intensity, which is also dependent on the solar zenithal angle. The mean diurnal VTEC shows a semiannual variation, with larger peaks in equinoxes for all years; no winter anomaly was observed, and in summer, there was no clear diurnal variation. The semiannual variation of the VTEC is also modulated by solar activity, with larger VTEC peaks when the solar activity was higher. Facultad de Ciencias Astronómicas y Geofísicas |
description |
The vertical total electron content (VTEC) obtained from 2004 to 2011 at Comandante Ferraz Brazilian Antarctic Station (62.1°S, 58.4°W) is analyzed to study the mean diurnal, seasonal and annual variations. The maximum daytime VTEC had an annual variation that decreased from 2004 to 2008, and then starting to increase in 2009, which followed the variation of the solar activity. The daily VTEC shows good linear correlation with solar radiation intensity, which is also dependent on the solar zenithal angle. The mean diurnal VTEC shows a semiannual variation, with larger peaks in equinoxes for all years; no winter anomaly was observed, and in summer, there was no clear diurnal variation. The semiannual variation of the VTEC is also modulated by solar activity, with larger VTEC peaks when the solar activity was higher. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-04 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/99989 |
url |
http://sedici.unlp.edu.ar/handle/10915/99989 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/23228 info:eu-repo/semantics/altIdentifier/url/http://www.annalsofgeophysics.eu/index.php/annals/article/view/6223 info:eu-repo/semantics/altIdentifier/issn/2037-416X info:eu-repo/semantics/altIdentifier/doi/10.4401/ag-6223 info:eu-repo/semantics/altIdentifier/hdl/11336/23228 |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf 1-5 |
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