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...

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Detalles Bibliográficos
Autores: Hysell, D. L., Chau Chong Shing, Jorge Luis, Huba, J. D.
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
format 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
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv 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
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:0992-7689
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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eu_rights_str_mv openAccess
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dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv European Geosciences Union (EGU)
publisher.none.fl_str_mv European Geosciences Union (EGU)
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
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spelling 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. 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