Topside measurements at Jicamarca during solar minimum
Descripción del Articulo
Long-pulse topside radar data acquired at Jicamarca and processed using full-profile analysis are compared to data processed using more conventional, range-gated approaches and with analytic and computational models. The salient features of the topside observations include a dramatic increase in the...
| Autores: | , , |
|---|---|
| Formato: | artículo |
| Fecha de Publicación: | 2009 |
| Institución: | Instituto Geofísico del Perú |
| Repositorio: | IGP-Institucional |
| Lenguaje: | inglés |
| OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/1966 |
| Enlace del recurso: | http://hdl.handle.net/20.500.12816/1966 https://doi.org/10.5194/angeo-27-427-2009 |
| Nivel de acceso: | acceso abierto |
| Materia: | Ionosphere Equatorial ionosphere Radar http://purl.org/pe-repo/ocde/ford#1.05.01 |
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| dc.title.none.fl_str_mv |
Topside measurements at Jicamarca during solar minimum |
| title |
Topside measurements at Jicamarca during solar minimum |
| spellingShingle |
Topside measurements at Jicamarca during solar minimum Hysell, D. L. Ionosphere Equatorial ionosphere Radar http://purl.org/pe-repo/ocde/ford#1.05.01 |
| title_short |
Topside measurements at Jicamarca during solar minimum |
| title_full |
Topside measurements at Jicamarca during solar minimum |
| title_fullStr |
Topside measurements at Jicamarca during solar minimum |
| title_full_unstemmed |
Topside measurements at Jicamarca during solar minimum |
| title_sort |
Topside measurements at Jicamarca during solar minimum |
| author |
Hysell, D. L. |
| author_facet |
Hysell, D. L. Chau Chong Shing, Jorge Luis Huba, J. D. |
| author_role |
author |
| author2 |
Chau Chong Shing, Jorge Luis Huba, J. D. |
| author2_role |
author author |
| dc.contributor.author.fl_str_mv |
Hysell, D. L. Chau Chong Shing, Jorge Luis Huba, J. D. |
| dc.subject.none.fl_str_mv |
Ionosphere Equatorial ionosphere Radar |
| topic |
Ionosphere Equatorial ionosphere Radar 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 |
Long-pulse topside radar data acquired at Jicamarca and processed using full-profile analysis are compared to data processed using more conventional, range-gated approaches and with analytic and computational models. The salient features of the topside observations include a dramatic increase in the Te/Ti temperature ratio above the F peak at dawn and a local minimum in the topside plasma temperature in the afternoon. The hydrogen ion fraction was found to exhibit hyperbolic tangent-shaped profiles that become shallow (gradually changing) above the O+-H+ transition height during the day. The profile shapes are generally consistent with diffusive equilibrium, although shallowing to the point of changes in inflection can only be accounted for by taking the effects of E×B drifts and meridional winds into account. The SAMI2 model demonstrates this as well as the substantial effect that drifts and winds can have on topside temperatures. Significant quiet-time variability in the topside composition and temperatures may be due to variability in the mechanical forcing. Correlations between topside measurements and magnetometer data at Jicamarca support this hypothesis. |
| publishDate |
2009 |
| dc.date.accessioned.none.fl_str_mv |
2018-07-19T16:00:00Z |
| dc.date.available.none.fl_str_mv |
2018-07-19T16:00:00Z |
| dc.date.issued.fl_str_mv |
2009-01-23 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
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article |
| dc.identifier.citation.none.fl_str_mv |
Hysell, D. L., Chau, J. L., & Huba, J. D. (2009). Topside measurements at Jicamarca during solar minimum.==$Annales Geophysicae, 27$==(1), 427-439. https://doi.org/10.5194/angeo-27-427-2009 |
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index-oti2018 |
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http://hdl.handle.net/20.500.12816/1966 |
| dc.identifier.journal.none.fl_str_mv |
Annales Geophysicae |
| dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.5194/angeo-27-427-2009 |
| identifier_str_mv |
Hysell, D. L., Chau, J. L., & Huba, J. D. (2009). Topside measurements at Jicamarca during solar minimum.==$Annales Geophysicae, 27$==(1), 427-439. https://doi.org/10.5194/angeo-27-427-2009 index-oti2018 Annales Geophysicae |
| url |
http://hdl.handle.net/20.500.12816/1966 https://doi.org/10.5194/angeo-27-427-2009 |
| dc.language.iso.none.fl_str_mv |
eng |
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eng |
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urn:issn:0992-7689 |
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info:eu-repo/semantics/openAccess |
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https://creativecommons.org/licences/by/4.0/ |
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openAccess |
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https://creativecommons.org/licences/by/4.0/ |
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application/pdf |
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European Geosciences Union (EGU) |
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European Geosciences Union (EGU) |
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reponame:IGP-Institucional instname:Instituto Geofísico del Perú instacron:IGP |
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Hysell, D. L.Chau Chong Shing, Jorge LuisHuba, J. D.2018-07-19T16:00:00Z2018-07-19T16:00:00Z2009-01-23Hysell, D. L., Chau, J. L., & Huba, J. D. (2009). Topside measurements at Jicamarca during solar minimum.==$Annales Geophysicae, 27$==(1), 427-439. https://doi.org/10.5194/angeo-27-427-2009index-oti2018http://hdl.handle.net/20.500.12816/1966Annales Geophysicaehttps://doi.org/10.5194/angeo-27-427-2009Long-pulse topside radar data acquired at Jicamarca and processed using full-profile analysis are compared to data processed using more conventional, range-gated approaches and with analytic and computational models. The salient features of the topside observations include a dramatic increase in the Te/Ti temperature ratio above the F peak at dawn and a local minimum in the topside plasma temperature in the afternoon. The hydrogen ion fraction was found to exhibit hyperbolic tangent-shaped profiles that become shallow (gradually changing) above the O+-H+ transition height during the day. The profile shapes are generally consistent with diffusive equilibrium, although shallowing to the point of changes in inflection can only be accounted for by taking the effects of E×B drifts and meridional winds into account. The SAMI2 model demonstrates this as well as the substantial effect that drifts and winds can have on topside temperatures. Significant quiet-time variability in the topside composition and temperatures may be due to variability in the mechanical forcing. Correlations between topside measurements and magnetometer data at Jicamarca support this hypothesis.Por paresapplication/pdfengEuropean Geosciences Union (EGU)urn:issn:0992-7689info:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/IonosphereEquatorial ionosphereRadarhttp://purl.org/pe-repo/ocde/ford#1.05.01Topside measurements at Jicamarca during solar minimuminfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALHysell_angeo-27-427-2009.pdfHysell_angeo-27-427-2009.pdfapplication/pdf1477903https://repositorio.igp.gob.pe/bitstreams/421a14ea-ad8e-4d57-83be-adbd641f98cc/download3741b032e12ccc2afea13be0aff3dd99MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/c7883c3c-489c-428a-b4f6-9abc9cc9bc83/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILHysell_angeo-27-427-2009.pdf.jpgHysell_angeo-27-427-2009.pdf.jpgIM Thumbnailimage/jpeg100183https://repositorio.igp.gob.pe/bitstreams/d3b927f7-4db8-472f-8125-8bd0b29521a4/download7d139c027793a1d82d4532d37afd39c1MD53TEXTHysell_angeo-27-427-2009.pdf.txtHysell_angeo-27-427-2009.pdf.txtExtracted texttext/plain53381https://repositorio.igp.gob.pe/bitstreams/f4424eef-f752-4fab-ba57-2ee65ad469cc/downloadc099d67d5e30b4ad2e3e438bb9ebcb31MD5420.500.12816/1966oai:repositorio.igp.gob.pe:20.500.12816/19662024-10-12 22:18:36.115https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.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).