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...
| Autores: | , , , , , |
|---|---|
| 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 |
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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 |
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http://hdl.handle.net/20.500.12816/2052 https://doi.org/10.1002/2014JA019963 |
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eng |
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eng |
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urn:issn:2169-9380 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
| dc.publisher.none.fl_str_mv |
American Geophysical Union |
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American Geophysical Union |
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Instituto Geofísico del Perú |
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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. 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.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccessEquatorial ionospherePlasma bubbleZonal plasma motionhttp://purl.org/pe-repo/ocde/ford#1.05.01The zonal motion of equatorial plasma bubbles relative to the background ionosphereinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALAAI0036.pdfAAI0036.pdfapplication/pdf2386719https://repositorio.igp.gob.pe/bitstreams/e9ed7d56-438c-4f8b-bd86-2f4c7c7ee52b/downloadafa316cc51e2e093f53f8a2f69631a08MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/cc8865cc-b664-42ed-a45d-a60aadb5f3f5/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILAAI0036.pdf.jpgAAI0036.pdf.jpgIM Thumbnailimage/jpeg109640https://repositorio.igp.gob.pe/bitstreams/e7f5d4ce-c66d-4702-bece-4d21c596bdc5/downloadb4b7deacbe3208edc156c87f9311c745MD53TEXTAAI0036.pdf.txtAAI0036.pdf.txtExtracted texttext/plain36877https://repositorio.igp.gob.pe/bitstreams/3c45f164-45b6-41e8-b478-ad6bd5310dd1/download36f4c6e8a4a912fedd7f49d4b074abefMD5420.500.12816/2052oai:repositorio.igp.gob.pe:20.500.12816/20522025-08-13 10:36:56.003open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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 |
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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).