Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?
Descripción del Articulo
Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Ou...
Autores: | , |
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Formato: | artículo |
Fecha de Publicación: | 2013 |
Institución: | Instituto Geofísico del Perú |
Repositorio: | IGP-Institucional |
Lenguaje: | inglés |
OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/3539 |
Enlace del recurso: | http://hdl.handle.net/20.500.12816/3539 https://doi.org/10.1002/grl.50693 |
Nivel de acceso: | acceso abierto |
Materia: | Equatorial ionosphere Irregularities bubbles Plasma http://purl.org/pe-repo/ocde/ford#1.05.01 |
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Kil, HyosubLee, Woo Kyoung2018-11-13T11:17:14Z2018-11-13T11:17:14Z2013-06-24Kil, H., & Lee, W. K. (2013). Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?.==$Geophysical Research Letters, 40$==(14), 3491-3495. https://doi.org/10.1002/grl.50693http://hdl.handle.net/20.500.12816/3539Geophysical Research Lettershttps://doi.org/10.1002/grl.50693Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Outage Forecasting System (C/NOFS) satellite on 31 December 2008, 28 July 2010, and 1 February 2011. On those days, BPDs are detected in the longitude regions where C/NOFS did not detect bubbles prior to the detection of BPDs. The coincident C/NOFS and radar observations over Jicamarca in Peru show the occurrence of BPDs at the time when backscatter echoes are absent and at the height below backscatter echoes. These observations indicate that bubbles are not a prerequisite for those BPDs. The detections of those BPDs can be explained by the uplift of the equatorial F region peak height above the satellite orbit.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:0094-8276info:eu-repo/semantics/openAccessEquatorial ionosphereIrregularities bubblesPlasmahttp://purl.org/pe-repo/ocde/ford#1.05.01Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?info:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-1-1-1495466428.pdfIGP-1-1-1-1495466428.pdfapplication/pdf470398https://repositorio.igp.gob.pe/bitstreams/7b3c2311-e3b9-4906-8d29-1b9cec72dc88/download86d45a4e4ea4c6e060ccd068d307d844MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8391https://repositorio.igp.gob.pe/bitstreams/3818c437-496f-49c7-b5f5-d43b9d936fe0/downloadef941c35636116525aadeaab7bbf4ca3MD52THUMBNAILIGP-1-1-1-1495466428.pdf.jpgIGP-1-1-1-1495466428.pdf.jpgIM Thumbnailimage/jpeg105320https://repositorio.igp.gob.pe/bitstreams/d379c534-1de7-4432-87fe-13f229fa27ff/downloadd9945f252992c83452c5d7f719c741d2MD53TEXTIGP-1-1-1-1495466428.pdf.txtIGP-1-1-1-1495466428.pdf.txtExtracted texttext/plain24309https://repositorio.igp.gob.pe/bitstreams/cb487f63-1abc-4552-87ad-570940042644/downloadacb25edf27cb660369a0ba6d509ea711MD5420.500.12816/3539oai:repositorio.igp.gob.pe:20.500.12816/35392025-08-13 09:44:41.35open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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 |
dc.title.none.fl_str_mv |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
title |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
spellingShingle |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? Kil, Hyosub Equatorial ionosphere Irregularities bubbles Plasma http://purl.org/pe-repo/ocde/ford#1.05.01 |
title_short |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
title_full |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
title_fullStr |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
title_full_unstemmed |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
title_sort |
Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
author |
Kil, Hyosub |
author_facet |
Kil, Hyosub Lee, Woo Kyoung |
author_role |
author |
author2 |
Lee, Woo Kyoung |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Kil, Hyosub Lee, Woo Kyoung |
dc.subject.none.fl_str_mv |
Equatorial ionosphere Irregularities bubbles Plasma |
topic |
Equatorial ionosphere Irregularities bubbles Plasma 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 |
Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Outage Forecasting System (C/NOFS) satellite on 31 December 2008, 28 July 2010, and 1 February 2011. On those days, BPDs are detected in the longitude regions where C/NOFS did not detect bubbles prior to the detection of BPDs. The coincident C/NOFS and radar observations over Jicamarca in Peru show the occurrence of BPDs at the time when backscatter echoes are absent and at the height below backscatter echoes. These observations indicate that bubbles are not a prerequisite for those BPDs. The detections of those BPDs can be explained by the uplift of the equatorial F region peak height above the satellite orbit. |
publishDate |
2013 |
dc.date.accessioned.none.fl_str_mv |
2018-11-13T11:17:14Z |
dc.date.available.none.fl_str_mv |
2018-11-13T11:17:14Z |
dc.date.issued.fl_str_mv |
2013-06-24 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
dc.identifier.citation.none.fl_str_mv |
Kil, H., & Lee, W. K. (2013). Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?.==$Geophysical Research Letters, 40$==(14), 3491-3495. https://doi.org/10.1002/grl.50693 |
dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/3539 |
dc.identifier.journal.none.fl_str_mv |
Geophysical Research Letters |
dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.1002/grl.50693 |
identifier_str_mv |
Kil, H., & Lee, W. K. (2013). Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?.==$Geophysical Research Letters, 40$==(14), 3491-3495. https://doi.org/10.1002/grl.50693 Geophysical Research Letters |
url |
http://hdl.handle.net/20.500.12816/3539 https://doi.org/10.1002/grl.50693 |
dc.language.iso.none.fl_str_mv |
eng |
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eng |
dc.relation.ispartof.none.fl_str_mv |
urn:issn:0094-8276 |
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 |
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IGP-Institucional |
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La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).