Ionospheric variations during January 2009 stratospheric sudden warming

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The stratospheric sudden warming peaking in January 2009 was the strongest and most prolonged on record. We report significant ionospheric variations is association with this event, which are especially pronounced at low latitudes. Large increase in the vertical drifts is observed at Jicamarca, disp...

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Detalles Bibliográficos
Autores: Goncharenko, L., Coster, A., Rideout, W., Chau Chong Shing, Jorge Luis, Liu, H. -L., Valladares, C. E.
Formato: objeto de conferencia
Fecha de Publicación:2009
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3638
Enlace del recurso:http://hdl.handle.net/20.500.12816/3638
Nivel de acceso:acceso abierto
Materia:Ionosphere
Seasonal variations
Stratosphere
Electron density
Electrons
http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
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spelling Goncharenko, L.Coster, A.Rideout, W.Chau Chong Shing, Jorge LuisLiu, H. -L.Valladares, C. E.2018-11-15T18:04:54Z2018-11-15T18:04:54Z2009http://hdl.handle.net/20.500.12816/3638The stratospheric sudden warming peaking in January 2009 was the strongest and most prolonged on record. We report significant ionospheric variations is association with this event, which are especially pronounced at low latitudes. Large increase in the vertical drifts is observed at Jicamarca, displaying 12-hour signature with upward drifts in the morning hours and downward drifts in the afternoon hours, with pattern persisting for several days. Analysis of GPS TEC data indicates that variations in electron density are observed in a large range of longitudes and latitudes. The entire daytime ionosphere is affected, with morning increase in low-latitude TEC exceeding 100% of the mean value, and afternoon decrease in TEC approaching ~50% of the mean value. These variations are consistent with ionospheric disturbances observed during other stratospheric warming events. We suggest the observed phenomena is related to planetary waves, which have a high amplitude level prior to the stratospheric warmings. Interaction of planetary waves with tides and modulation of tides can lead to changes in the low-latitude electric field through the wind dynamo process, which in turn is responsible for a largescale redistribution of ionospheric electron density.MIT Haystack Observatory; NCAR -Boston Universityapplication/pdfengInstituto Geofísico del Perúinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/IonosphereSeasonal variationsStratosphereElectron densityElectronshttp://purl.org/pe-repo/ocde/ford#1.05.01http://purl.org/pe-repo/ocde/ford#1.05.00Ionospheric variations during January 2009 stratospheric sudden warminginfo:eu-repo/semantics/conferenceObjectreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALgoncharenko2009.pdfgoncharenko2009.pdfapplication/pdf1406342https://repositorio.igp.gob.pe/bitstreams/1526910b-7ad1-4a60-a37e-97ba0cb81d6a/download49dcbc7f5bb989b3d4ab8af992f4556bMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8393https://repositorio.igp.gob.pe/bitstreams/540fd256-31f2-4f7d-b699-fdc7c23b8fc1/downloadf6e2e38ecabbf5c802f4b273da8f9399MD52THUMBNAILgoncharenko2009.pdf.jpggoncharenko2009.pdf.jpgIM Thumbnailimage/jpeg104934https://repositorio.igp.gob.pe/bitstreams/75e28535-7a30-4842-9922-10930575ba5c/download1f5e34958c3398bbc392826396511639MD53TEXTgoncharenko2009.pdf.txtgoncharenko2009.pdf.txtExtracted texttext/plain5564https://repositorio.igp.gob.pe/bitstreams/ae9349de-3999-4b6e-b60e-545707051893/downloadb51ac31e3d8b45ffcf5f43ec8dd8a0dfMD5420.500.12816/3638oai:repositorio.igp.gob.pe:20.500.12816/36382021-03-10 12:01:46.479https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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
dc.title.es_ES.fl_str_mv Ionospheric variations during January 2009 stratospheric sudden warming
title Ionospheric variations during January 2009 stratospheric sudden warming
spellingShingle Ionospheric variations during January 2009 stratospheric sudden warming
Goncharenko, L.
Ionosphere
Seasonal variations
Stratosphere
Electron density
Electrons
http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
title_short Ionospheric variations during January 2009 stratospheric sudden warming
title_full Ionospheric variations during January 2009 stratospheric sudden warming
title_fullStr Ionospheric variations during January 2009 stratospheric sudden warming
title_full_unstemmed Ionospheric variations during January 2009 stratospheric sudden warming
title_sort Ionospheric variations during January 2009 stratospheric sudden warming
author Goncharenko, L.
author_facet Goncharenko, L.
Coster, A.
Rideout, W.
Chau Chong Shing, Jorge Luis
Liu, H. -L.
Valladares, C. E.
author_role author
author2 Coster, A.
Rideout, W.
Chau Chong Shing, Jorge Luis
Liu, H. -L.
Valladares, C. E.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Goncharenko, L.
Coster, A.
Rideout, W.
Chau Chong Shing, Jorge Luis
Liu, H. -L.
Valladares, C. E.
dc.subject.es_ES.fl_str_mv Ionosphere
Seasonal variations
Stratosphere
Electron density
Electrons
topic Ionosphere
Seasonal variations
Stratosphere
Electron density
Electrons
http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
dc.subject.ocde.es_ES.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
description The stratospheric sudden warming peaking in January 2009 was the strongest and most prolonged on record. We report significant ionospheric variations is association with this event, which are especially pronounced at low latitudes. Large increase in the vertical drifts is observed at Jicamarca, displaying 12-hour signature with upward drifts in the morning hours and downward drifts in the afternoon hours, with pattern persisting for several days. Analysis of GPS TEC data indicates that variations in electron density are observed in a large range of longitudes and latitudes. The entire daytime ionosphere is affected, with morning increase in low-latitude TEC exceeding 100% of the mean value, and afternoon decrease in TEC approaching ~50% of the mean value. These variations are consistent with ionospheric disturbances observed during other stratospheric warming events. We suggest the observed phenomena is related to planetary waves, which have a high amplitude level prior to the stratospheric warmings. Interaction of planetary waves with tides and modulation of tides can lead to changes in the low-latitude electric field through the wind dynamo process, which in turn is responsible for a largescale redistribution of ionospheric electron density.
publishDate 2009
dc.date.accessioned.none.fl_str_mv 2018-11-15T18:04:54Z
dc.date.available.none.fl_str_mv 2018-11-15T18:04:54Z
dc.date.issued.fl_str_mv 2009
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dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/3638
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dc.language.iso.es_ES.fl_str_mv eng
language eng
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dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv Instituto Geofísico del Perú
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