Altitudinal dependence of evening equatorial F region vertical plasma drifts

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We use Jicamarca incoherent scatter radar measurements to study for the first time the altitudinal variations of late afternoon and early night equatorial F region vertical plasma drifts. We also present the initial vertical drift measurements over the altitudinal range from about 200 to 2000 km. Th...

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Detalles Bibliográficos
Autores: Fejer, B. G., Hui, D., Chau Chong Shing, Jorge Luis, Kudeki, E.
Formato: artículo
Fecha de Publicación:2014
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3593
Enlace del recurso:http://hdl.handle.net/20.500.12816/3593
https://doi.org/10.1002/2014JA019949
Nivel de acceso:acceso abierto
Materia:Electric fields
Equatorial ionosphere
Ionospheric electrodynamics
http://purl.org/pe-repo/ocde/ford#1.05.01
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spelling Fejer, B. G.Hui, D.Chau Chong Shing, Jorge LuisKudeki, E.2018-11-14T15:29:34Z2018-11-14T15:29:34Z2014-06-06Fejer, B. G., Hui, D., Chau, J. L., & Kudeki, E. (2014). Altitudinal dependence of evening equatorial F region vertical plasma drifts.==$Journal of Geophysical Research: Space Physics, 119$==(7), 5877-5890. https://doi.org/10.1002/2014JA019949http://hdl.handle.net/20.500.12816/3593Journal of Geophysical Research: Space Physicshttps://doi.org/10.1002/2014JA019949We use Jicamarca incoherent scatter radar measurements to study for the first time the altitudinal variations of late afternoon and early night equatorial F region vertical plasma drifts. We also present the initial vertical drift measurements over the altitudinal range from about 200 to 2000 km. These data show that the afternoon drifts decrease weakly with altitude. Near their evening prereversal enhancements, the vertical drifts generally increase with altitude below about the F layer peak, decrease with height near the F layer peak and above, and are nearly height independent in the (solar flux dependent) topside ionosphere. The transition altitudes from height‐decreasing to height‐independent evening upward drifts decrease with altitude from solar maximum to solar minimum. After their reversal to downward, the vertical drifts do not change much with height. The altitudinal dependence of the evening vertical drifts has large day‐to‐day variability and is closely related to the time dependence of the zonal drifts, as expected from the curl‐free electric field condition.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccessElectric fieldsEquatorial ionosphereIonospheric electrodynamicshttp://purl.org/pe-repo/ocde/ford#1.05.01Altitudinal dependence of evening equatorial F region vertical plasma driftsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-1-1-1466402003.pdfIGP-1-1-1-1466402003.pdfapplication/pdf1823261https://repositorio.igp.gob.pe/bitstreams/8682e51c-375c-4bd3-be4f-d314b3f2ef2a/download65c0d4278bf8b28433d399084c34ad57MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8391https://repositorio.igp.gob.pe/bitstreams/5eaf6c93-a0e7-4070-a693-feda02a1ecec/downloadef941c35636116525aadeaab7bbf4ca3MD52THUMBNAILIGP-1-1-1-1466402003.pdf.jpgIGP-1-1-1-1466402003.pdf.jpgIM Thumbnailimage/jpeg102736https://repositorio.igp.gob.pe/bitstreams/b1b9b73a-749e-4b0b-968f-0b86dc5e21ba/downloadaa0cab3e7bbdf4ca05c291db7d6daa23MD53TEXTIGP-1-1-1-1466402003.pdf.txtIGP-1-1-1-1466402003.pdf.txtExtracted texttext/plain52200https://repositorio.igp.gob.pe/bitstreams/216702eb-435e-4e9d-a2aa-3452cf82047d/download91b35aa9042d15b98f854dc9d11dcf9cMD5420.500.12816/3593oai:repositorio.igp.gob.pe:20.500.12816/35932025-08-14 10:33:03.879restrictedhttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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
dc.title.none.fl_str_mv Altitudinal dependence of evening equatorial F region vertical plasma drifts
title Altitudinal dependence of evening equatorial F region vertical plasma drifts
spellingShingle Altitudinal dependence of evening equatorial F region vertical plasma drifts
Fejer, B. G.
Electric fields
Equatorial ionosphere
Ionospheric electrodynamics
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Altitudinal dependence of evening equatorial F region vertical plasma drifts
title_full Altitudinal dependence of evening equatorial F region vertical plasma drifts
title_fullStr Altitudinal dependence of evening equatorial F region vertical plasma drifts
title_full_unstemmed Altitudinal dependence of evening equatorial F region vertical plasma drifts
title_sort Altitudinal dependence of evening equatorial F region vertical plasma drifts
author Fejer, B. G.
author_facet Fejer, B. G.
Hui, D.
Chau Chong Shing, Jorge Luis
Kudeki, E.
author_role author
author2 Hui, D.
Chau Chong Shing, Jorge Luis
Kudeki, E.
author2_role author
author
author
dc.contributor.author.fl_str_mv Fejer, B. G.
Hui, D.
Chau Chong Shing, Jorge Luis
Kudeki, E.
dc.subject.none.fl_str_mv Electric fields
Equatorial ionosphere
Ionospheric electrodynamics
topic Electric fields
Equatorial ionosphere
Ionospheric electrodynamics
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 We use Jicamarca incoherent scatter radar measurements to study for the first time the altitudinal variations of late afternoon and early night equatorial F region vertical plasma drifts. We also present the initial vertical drift measurements over the altitudinal range from about 200 to 2000 km. These data show that the afternoon drifts decrease weakly with altitude. Near their evening prereversal enhancements, the vertical drifts generally increase with altitude below about the F layer peak, decrease with height near the F layer peak and above, and are nearly height independent in the (solar flux dependent) topside ionosphere. The transition altitudes from height‐decreasing to height‐independent evening upward drifts decrease with altitude from solar maximum to solar minimum. After their reversal to downward, the vertical drifts do not change much with height. The altitudinal dependence of the evening vertical drifts has large day‐to‐day variability and is closely related to the time dependence of the zonal drifts, as expected from the curl‐free electric field condition.
publishDate 2014
dc.date.accessioned.none.fl_str_mv 2018-11-14T15:29:34Z
dc.date.available.none.fl_str_mv 2018-11-14T15:29:34Z
dc.date.issued.fl_str_mv 2014-06-06
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Fejer, B. G., Hui, D., Chau, J. L., & Kudeki, E. (2014). Altitudinal dependence of evening equatorial F region vertical plasma drifts.==$Journal of Geophysical Research: Space Physics, 119$==(7), 5877-5890. https://doi.org/10.1002/2014JA019949
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/3593
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1002/2014JA019949
identifier_str_mv Fejer, B. G., Hui, D., Chau, J. L., & Kudeki, E. (2014). Altitudinal dependence of evening equatorial F region vertical plasma drifts.==$Journal of Geophysical Research: Space Physics, 119$==(7), 5877-5890. https://doi.org/10.1002/2014JA019949
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/3593
https://doi.org/10.1002/2014JA019949
dc.language.iso.none.fl_str_mv eng
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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
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