Upwelling: a unit of disturbance in equatorial spread F

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Plasma structure in the nighttime equatorial F layer, often referred to as equatorial spread F (ESF), is not uniformly distributed, either in time or in space. Observations indicate that ESF in the bottomside F layer takes the form of patches; plasma structure within the F layer takes the form of lo...

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Detalles Bibliográficos
Autor: Tsunoda, Roland T.
Formato: artículo
Fecha de Publicación:2015
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3611
Enlace del recurso:http://hdl.handle.net/20.500.12816/3611
https://doi.org/10.1186/s40645-015-0038-5
Nivel de acceso:acceso abierto
Materia:Equatorial spread F
F-region plasma structure
Equatorial ionosphere
Equatorial plasma bubbles
Deep convective activity in troposphere
Atmospheric gravity waves
http://purl.org/pe-repo/ocde/ford#1.05.01
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spelling Tsunoda, Roland T.2018-11-14T17:58:10Z2018-11-14T17:58:10Z2015-04-23Tsunoda, R. T. (2015). Upwelling: a unit of disturbance in equatorial spread F.==$Progress in Earth and Planetary Science, 2$==(9), 1-14. https://doi.org/10.1186/s40645-015-0038-5http://hdl.handle.net/20.500.12816/3611Progress in Earth and Planetary Sciencehttps://doi.org/10.1186/s40645-015-0038-5Plasma structure in the nighttime equatorial F layer, often referred to as equatorial spread F (ESF), is not uniformly distributed, either in time or in space. Observations indicate that ESF in the bottomside F layer takes the form of patches; plasma structure within the F layer takes the form of localized plasma depletions, called equatorial plasma bubbles (EPBs), which tend to occur in clusters. Another observed feature is an upwelling, which has been described as a localized, upward modulation of isodensity contours in the bottomside F layer. Interestingly, zonal widths of ESF patches, EPB clusters, and upwellings are similar. Moreover, all display an east-west asymmetry. The objective of this paper is to show, for the first time, that an ESF patch is the bottomside counterpart of an EPB cluster, and that both are products of the electrodynamical process that takes place within an upwelling. The process can be described as having three phases: (1) amplification of upwelling amplitude during the post-sunset rise of the F layer, (2) launching of the first EPB of the evening, from crest of the upwelling, and (3) structuring of plasma within the upwelling. Hence, an upwelling, whose presence is responsible for the formation of ESF patches and EPB clusters, can be envisioned as a unit of disturbance that occurs in the nighttime equatorial ionosphere.Por paresapplication/pdfengSpringerOpenurn:issn:2197-4284info:eu-repo/semantics/openAccessEquatorial spread FF-region plasma structureEquatorial ionosphereEquatorial plasma bubblesDeep convective activity in troposphereAtmospheric gravity waveshttp://purl.org/pe-repo/ocde/ford#1.05.01Upwelling: a unit of disturbance in equatorial spread Finfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-1-1-1432156058.pdfIGP-1-1-1-1432156058.pdfapplication/pdf3990759https://repositorio.igp.gob.pe/bitstreams/5d9ac4e7-24a5-4eda-8ff6-6c8e14482941/download7632d367a04a5f15cdef64fbf8dd9e24MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8391https://repositorio.igp.gob.pe/bitstreams/bc408e2d-fe91-4887-b462-2d943503411d/downloadef941c35636116525aadeaab7bbf4ca3MD52THUMBNAILIGP-1-1-1-1432156058.pdf.jpgIGP-1-1-1-1432156058.pdf.jpgIM Thumbnailimage/jpeg160035https://repositorio.igp.gob.pe/bitstreams/c8457681-ee43-4b86-a29b-cc7e5c3b1761/download51beca7fa936e9a938ec969ae8e56fd3MD53TEXTIGP-1-1-1-1432156058.pdf.txtIGP-1-1-1-1432156058.pdf.txtExtracted texttext/plain69430https://repositorio.igp.gob.pe/bitstreams/b5bef04e-de42-4042-94af-fe7b4182a787/download94413238d1f70fe3ef7ce3cdad10502fMD5420.500.12816/3611oai:repositorio.igp.gob.pe:20.500.12816/36112025-08-14 11:15:42.513open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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
dc.title.none.fl_str_mv Upwelling: a unit of disturbance in equatorial spread F
title Upwelling: a unit of disturbance in equatorial spread F
spellingShingle Upwelling: a unit of disturbance in equatorial spread F
Tsunoda, Roland T.
Equatorial spread F
F-region plasma structure
Equatorial ionosphere
Equatorial plasma bubbles
Deep convective activity in troposphere
Atmospheric gravity waves
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Upwelling: a unit of disturbance in equatorial spread F
title_full Upwelling: a unit of disturbance in equatorial spread F
title_fullStr Upwelling: a unit of disturbance in equatorial spread F
title_full_unstemmed Upwelling: a unit of disturbance in equatorial spread F
title_sort Upwelling: a unit of disturbance in equatorial spread F
author Tsunoda, Roland T.
author_facet Tsunoda, Roland T.
author_role author
dc.contributor.author.fl_str_mv Tsunoda, Roland T.
dc.subject.none.fl_str_mv Equatorial spread F
F-region plasma structure
Equatorial ionosphere
Equatorial plasma bubbles
Deep convective activity in troposphere
Atmospheric gravity waves
topic Equatorial spread F
F-region plasma structure
Equatorial ionosphere
Equatorial plasma bubbles
Deep convective activity in troposphere
Atmospheric gravity waves
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 Plasma structure in the nighttime equatorial F layer, often referred to as equatorial spread F (ESF), is not uniformly distributed, either in time or in space. Observations indicate that ESF in the bottomside F layer takes the form of patches; plasma structure within the F layer takes the form of localized plasma depletions, called equatorial plasma bubbles (EPBs), which tend to occur in clusters. Another observed feature is an upwelling, which has been described as a localized, upward modulation of isodensity contours in the bottomside F layer. Interestingly, zonal widths of ESF patches, EPB clusters, and upwellings are similar. Moreover, all display an east-west asymmetry. The objective of this paper is to show, for the first time, that an ESF patch is the bottomside counterpart of an EPB cluster, and that both are products of the electrodynamical process that takes place within an upwelling. The process can be described as having three phases: (1) amplification of upwelling amplitude during the post-sunset rise of the F layer, (2) launching of the first EPB of the evening, from crest of the upwelling, and (3) structuring of plasma within the upwelling. Hence, an upwelling, whose presence is responsible for the formation of ESF patches and EPB clusters, can be envisioned as a unit of disturbance that occurs in the nighttime equatorial ionosphere.
publishDate 2015
dc.date.accessioned.none.fl_str_mv 2018-11-14T17:58:10Z
dc.date.available.none.fl_str_mv 2018-11-14T17:58:10Z
dc.date.issued.fl_str_mv 2015-04-23
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Tsunoda, R. T. (2015). Upwelling: a unit of disturbance in equatorial spread F.==$Progress in Earth and Planetary Science, 2$==(9), 1-14. https://doi.org/10.1186/s40645-015-0038-5
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/3611
dc.identifier.journal.none.fl_str_mv Progress in Earth and Planetary Science
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1186/s40645-015-0038-5
identifier_str_mv Tsunoda, R. T. (2015). Upwelling: a unit of disturbance in equatorial spread F.==$Progress in Earth and Planetary Science, 2$==(9), 1-14. https://doi.org/10.1186/s40645-015-0038-5
Progress in Earth and Planetary Science
url http://hdl.handle.net/20.500.12816/3611
https://doi.org/10.1186/s40645-015-0038-5
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dc.publisher.none.fl_str_mv SpringerOpen
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