The zonal motion of equatorial plasma bubbles relative to the background ionosphere

Descripción del Articulo

The zonal motions of plasmas inside equatorial plasma bubbles are different from those in the background ionosphere. The difference was explained in terms of the tilt of bubbles by recent studies, but observational evidence of this hypothesis has not yet been provided. We examine this hypothesis and...

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Detalles Bibliográficos
Autores: Kil, Hyosub, Lee, Woo Kyoung, Kwak, Young-Sil, Zhang, Yongliang, Paxton, Larry J., Milla, Marco
Formato: artículo
Fecha de Publicación:2014
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/2052
Enlace del recurso:http://hdl.handle.net/20.500.12816/2052
https://doi.org/10.1002/2014JA019963
Nivel de acceso:acceso abierto
Materia:Equatorial ionosphere
Plasma bubble
Zonal plasma motion
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv The zonal motion of equatorial plasma bubbles relative to the background ionosphere
title The zonal motion of equatorial plasma bubbles relative to the background ionosphere
spellingShingle The zonal motion of equatorial plasma bubbles relative to the background ionosphere
Kil, Hyosub
Equatorial ionosphere
Plasma bubble
Zonal plasma motion
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short The zonal motion of equatorial plasma bubbles relative to the background ionosphere
title_full The zonal motion of equatorial plasma bubbles relative to the background ionosphere
title_fullStr The zonal motion of equatorial plasma bubbles relative to the background ionosphere
title_full_unstemmed The zonal motion of equatorial plasma bubbles relative to the background ionosphere
title_sort The zonal motion of equatorial plasma bubbles relative to the background ionosphere
author Kil, Hyosub
author_facet Kil, Hyosub
Lee, Woo Kyoung
Kwak, Young-Sil
Zhang, Yongliang
Paxton, Larry J.
Milla, Marco
author_role author
author2 Lee, Woo Kyoung
Kwak, Young-Sil
Zhang, Yongliang
Paxton, Larry J.
Milla, Marco
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Kil, Hyosub
Lee, Woo Kyoung
Kwak, Young-Sil
Zhang, Yongliang
Paxton, Larry J.
Milla, Marco
dc.subject.none.fl_str_mv Equatorial ionosphere
Plasma bubble
Zonal plasma motion
topic Equatorial ionosphere
Plasma bubble
Zonal plasma motion
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 The zonal motions of plasmas inside equatorial plasma bubbles are different from those in the background ionosphere. The difference was explained in terms of the tilt of bubbles by recent studies, but observational evidence of this hypothesis has not yet been provided. We examine this hypothesis and, at the same time, look for an alternative explanation on the basis of the coincident satellite and radar observations over Jicamarca (11.95°S, 76.87°W) in Peru. In the observations at premidnight by the first Republic of China satellite (altitude: 600 km, inclination: 35°), plasmas inside bubbles drift westward relative to ambient plasmas. The same phenomenon is identified by radar observations. However, the relative westward plasma motions inside bubbles occur regardless of the tilt of bubbles, and therefore, the tilt is not the primary cause of the deviation of the plasma motions inside bubbles. The zonal plasma motions in the topside are characterized by systematic eastward drifts, whereas the zonal motions of plasmas in the bottomside backscatter layer show a mixture of eastward and westward drifts. The zonal plasma motions inside backscatter plumes resemble those in the bottomside backscatter layer. These observations indicate that plasmas inside bubbles maintain the properties of the zonal plasma motions in the bottomside where the bubbles originate. With this assumption, the deviation of the zonal motions of plasmas inside bubbles from those of ambient plasmas is understood in terms of the difference of the zonal plasma flows in the bottomside and topside.
publishDate 2014
dc.date.accessioned.none.fl_str_mv 2018-07-24T13:22:26Z
dc.date.available.none.fl_str_mv 2018-07-24T13:22:26Z
dc.date.issued.fl_str_mv 2014-07-09
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., Kwak, Y.-S., Zhang, Y., Paxton, L. J., & Milla, M. (2014). The zonal motion of equatorial plasma bubbles relative to the background ionosphere.==$Journal of Geophysical Research: Space Physics, 119$==(7), 5943-5950. https://doi.org/10.1002/2014JA019963
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/2052
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1002/2014JA019963
identifier_str_mv Kil, H., Lee, W. K., Kwak, Y.-S., Zhang, Y., Paxton, L. J., & Milla, M. (2014). The zonal motion of equatorial plasma bubbles relative to the background ionosphere.==$Journal of Geophysical Research: Space Physics, 119$==(7), 5943-5950. https://doi.org/10.1002/2014JA019963
index-oti2018
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/2052
https://doi.org/10.1002/2014JA019963
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
reponame_str IGP-Institucional
collection IGP-Institucional
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spelling Kil, HyosubLee, Woo KyoungKwak, Young-SilZhang, YongliangPaxton, Larry J.Milla, Marco2018-07-24T13:22:26Z2018-07-24T13:22:26Z2014-07-09Kil, H., Lee, W. K., Kwak, Y.-S., Zhang, Y., Paxton, L. J., & Milla, M. (2014). The zonal motion of equatorial plasma bubbles relative to the background ionosphere.==$Journal of Geophysical Research: Space Physics, 119$==(7), 5943-5950. https://doi.org/10.1002/2014JA019963index-oti2018http://hdl.handle.net/20.500.12816/2052Journal of Geophysical Research: Space Physicshttps://doi.org/10.1002/2014JA019963The zonal motions of plasmas inside equatorial plasma bubbles are different from those in the background ionosphere. The difference was explained in terms of the tilt of bubbles by recent studies, but observational evidence of this hypothesis has not yet been provided. We examine this hypothesis and, at the same time, look for an alternative explanation on the basis of the coincident satellite and radar observations over Jicamarca (11.95°S, 76.87°W) in Peru. In the observations at premidnight by the first Republic of China satellite (altitude: 600 km, inclination: 35°), plasmas inside bubbles drift westward relative to ambient plasmas. The same phenomenon is identified by radar observations. However, the relative westward plasma motions inside bubbles occur regardless of the tilt of bubbles, and therefore, the tilt is not the primary cause of the deviation of the plasma motions inside bubbles. The zonal plasma motions in the topside are characterized by systematic eastward drifts, whereas the zonal motions of plasmas in the bottomside backscatter layer show a mixture of eastward and westward drifts. The zonal plasma motions inside backscatter plumes resemble those in the bottomside backscatter layer. These observations indicate that plasmas inside bubbles maintain the properties of the zonal plasma motions in the bottomside where the bubbles originate. 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