Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms

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Ionospheric observations from the ground‐based GPS receiver network, CHAMP and GRACE satellites and ionosondes were used to examine topside and bottomside ionospheric variations at low and middle latitudes over the Pacific and American sectors during the October 2003 superstorms. The latitudinal var...

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Detalles Bibliográficos
Autores: Lei, Jiuhou, Zhu, Qingyu, Wang, Wenbin, Burns, Alan G., Zhao, Biqiang, Luan, Xiaoli, Zhong, Jiahao, Dou, Xiankang
Formato: artículo
Fecha de Publicación:2015
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3698
Enlace del recurso:http://hdl.handle.net/20.500.12816/3698
https://doi.org/10.1002/2015JA021310
Nivel de acceso:acceso abierto
Materia:Topside ionosphere
Ionospheric storms
Prompt penetration electric fields
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
title Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
spellingShingle Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
Lei, Jiuhou
Topside ionosphere
Ionospheric storms
Prompt penetration electric fields
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
title_full Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
title_fullStr Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
title_full_unstemmed Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
title_sort Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms
author Lei, Jiuhou
author_facet Lei, Jiuhou
Zhu, Qingyu
Wang, Wenbin
Burns, Alan G.
Zhao, Biqiang
Luan, Xiaoli
Zhong, Jiahao
Dou, Xiankang
author_role author
author2 Zhu, Qingyu
Wang, Wenbin
Burns, Alan G.
Zhao, Biqiang
Luan, Xiaoli
Zhong, Jiahao
Dou, Xiankang
author2_role author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Lei, Jiuhou
Zhu, Qingyu
Wang, Wenbin
Burns, Alan G.
Zhao, Biqiang
Luan, Xiaoli
Zhong, Jiahao
Dou, Xiankang
dc.subject.none.fl_str_mv Topside ionosphere
Ionospheric storms
Prompt penetration electric fields
topic Topside ionosphere
Ionospheric storms
Prompt penetration electric fields
http://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.none.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
description Ionospheric observations from the ground‐based GPS receiver network, CHAMP and GRACE satellites and ionosondes were used to examine topside and bottomside ionospheric variations at low and middle latitudes over the Pacific and American sectors during the October 2003 superstorms. The latitudinal variation and the storm time response of the ground‐based GPS total electron content (TEC) were generally consistent with those of the CHAMP and GRACE up‐looking TEC. The TECs at heights below the satellite altitudes during the main phases were comparable to, or even less than, the quiet time values. However, the storm time CHAMP and GRACE up‐looking TECs showed profound increases at low and middle latitudes. The ground‐based TEC and ionosonde data were also combined to study the TEC variations below and above the F2 peak height (hmF2). The topside TECs above hmF2 at low and middle latitudes showed significant increases during storm time; however, the bottomside TEC below hmF2 did not show so obvious changes. Consequently, the bottomside ionosphere made only a minor contribution to the ionospheric positive phase seen in the total TEC at low and middle latitudes. Moreover, at middle latitudes F2 peak electron densities during storm time did not have the obvious enhancements that were seen in both the ground‐based and topside TECs, although they were accompanied by increases of hmF2. Therefore, storm time TEC changes are not necessarily related to changes in ionospheric peak densities. Our results suggest that TEC increases at low and middle latitudes are also associated with effective plasma scale height variations during storms.
publishDate 2015
dc.date.accessioned.none.fl_str_mv 2018-11-19T15:43:56Z
dc.date.available.none.fl_str_mv 2018-11-19T15:43:56Z
dc.date.issued.fl_str_mv 2015-07-14
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Lei, J., Zhu, Q., Wang, W., Burns, A. G., Zhao, B., Luan, X., ... Dou, X. (2015). Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms.==$Journal of Geophysical Research: Space Physics, 120$==(8), 6974-6986. https://doi.org/10.1002/2015JA021310
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/3698
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1002/2015JA021310
identifier_str_mv Lei, J., Zhu, Q., Wang, W., Burns, A. G., Zhao, B., Luan, X., ... Dou, X. (2015). Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms.==$Journal of Geophysical Research: Space Physics, 120$==(8), 6974-6986. https://doi.org/10.1002/2015JA021310
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/3698
https://doi.org/10.1002/2015JA021310
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:2169-9380
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 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:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
institution IGP
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collection IGP-Institucional
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spelling Lei, JiuhouZhu, QingyuWang, WenbinBurns, Alan G.Zhao, BiqiangLuan, XiaoliZhong, JiahaoDou, Xiankang2018-11-19T15:43:56Z2018-11-19T15:43:56Z2015-07-14Lei, J., Zhu, Q., Wang, W., Burns, A. G., Zhao, B., Luan, X., ... Dou, X. (2015). Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstorms.==$Journal of Geophysical Research: Space Physics, 120$==(8), 6974-6986. https://doi.org/10.1002/2015JA021310http://hdl.handle.net/20.500.12816/3698Journal of Geophysical Research: Space Physicshttps://doi.org/10.1002/2015JA021310Ionospheric observations from the ground‐based GPS receiver network, CHAMP and GRACE satellites and ionosondes were used to examine topside and bottomside ionospheric variations at low and middle latitudes over the Pacific and American sectors during the October 2003 superstorms. The latitudinal variation and the storm time response of the ground‐based GPS total electron content (TEC) were generally consistent with those of the CHAMP and GRACE up‐looking TEC. The TECs at heights below the satellite altitudes during the main phases were comparable to, or even less than, the quiet time values. However, the storm time CHAMP and GRACE up‐looking TECs showed profound increases at low and middle latitudes. The ground‐based TEC and ionosonde data were also combined to study the TEC variations below and above the F2 peak height (hmF2). The topside TECs above hmF2 at low and middle latitudes showed significant increases during storm time; however, the bottomside TEC below hmF2 did not show so obvious changes. Consequently, the bottomside ionosphere made only a minor contribution to the ionospheric positive phase seen in the total TEC at low and middle latitudes. Moreover, at middle latitudes F2 peak electron densities during storm time did not have the obvious enhancements that were seen in both the ground‐based and topside TECs, although they were accompanied by increases of hmF2. Therefore, storm time TEC changes are not necessarily related to changes in ionospheric peak densities. Our results suggest that TEC increases at low and middle latitudes are also associated with effective plasma scale height variations during storms.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccessTopside ionosphereIonospheric stormsPrompt penetration electric fieldshttp://purl.org/pe-repo/ocde/ford#1.05.01Response of the topside and bottomside ionosphere at low and middle latitudes to the October 2003 superstormsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-1-1-1495144287.pdfIGP-1-1-1-1495144287.pdfapplication/pdf2829278https://repositorio.igp.gob.pe/bitstreams/166396f0-421b-45ff-beb7-e93a2eb5cf73/download4a011569635e4d2fb1249d45f55db21dMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8391https://repositorio.igp.gob.pe/bitstreams/4e3697e0-39ac-4ee8-a60f-b0a61b5985ed/downloadef941c35636116525aadeaab7bbf4ca3MD52THUMBNAILIGP-1-1-1-1495144287.pdf.jpgIGP-1-1-1-1495144287.pdf.jpgIM Thumbnailimage/jpeg106115https://repositorio.igp.gob.pe/bitstreams/8b3d5fb5-7492-4f11-91a6-f47bdaa57607/download128a4b93f7dd9b74cf6b51d3bf499befMD53TEXTIGP-1-1-1-1495144287.pdf.txtIGP-1-1-1-1495144287.pdf.txtExtracted texttext/plain44199https://repositorio.igp.gob.pe/bitstreams/2811a43a-76fe-494c-8f79-1d2f1b11b955/download8ce134558b6b2b326543968e2c6dc760MD5420.500.12816/3698oai:repositorio.igp.gob.pe:20.500.12816/36982025-08-13 11:02:49.08open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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