Early morning equatorial ionization anomaly from GOLD observations

Descripción del Articulo

During geomagnetically quiet and solar minimum conditions, spatial variations of the early morning thermosphere‐ionosphere (TI) system are expected to be mainly governed by wave dynamics. To study the postmidnight dynamical coupling, we investigated the early morning equatorial ionization anomaly (E...

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Detalles Bibliográficos
Autores: Laskar, F. I., Eastes, R. W., Martinis, C. R., Daniell, R. E., Pedatella, N. M., Burns, A. G., McClintock, W., Goncharenko, L. P., Coster, A., Milla, Marco, Wang, W., Valladares, C. E., Codrescu, M. V.
Formato: artículo
Fecha de Publicación:2020
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/4917
Enlace del recurso:http://hdl.handle.net/20.500.12816/4917
https://doi.org/10.1029/2019JA027487
Nivel de acceso:acceso abierto
Materia:Airglow
Total electron content
Thermosphere‐ionosphere dynamics
Equatorial ionization anomaly
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv Early morning equatorial ionization anomaly from GOLD observations
title Early morning equatorial ionization anomaly from GOLD observations
spellingShingle Early morning equatorial ionization anomaly from GOLD observations
Laskar, F. I.
Airglow
Total electron content
Thermosphere‐ionosphere dynamics
Equatorial ionization anomaly
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Early morning equatorial ionization anomaly from GOLD observations
title_full Early morning equatorial ionization anomaly from GOLD observations
title_fullStr Early morning equatorial ionization anomaly from GOLD observations
title_full_unstemmed Early morning equatorial ionization anomaly from GOLD observations
title_sort Early morning equatorial ionization anomaly from GOLD observations
author Laskar, F. I.
author_facet Laskar, F. I.
Eastes, R. W.
Martinis, C. R.
Daniell, R. E.
Pedatella, N. M.
Burns, A. G.
McClintock, W.
Goncharenko, L. P.
Coster, A.
Milla, Marco
Wang, W.
Valladares, C. E.
Codrescu, M. V.
author_role author
author2 Eastes, R. W.
Martinis, C. R.
Daniell, R. E.
Pedatella, N. M.
Burns, A. G.
McClintock, W.
Goncharenko, L. P.
Coster, A.
Milla, Marco
Wang, W.
Valladares, C. E.
Codrescu, M. V.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Laskar, F. I.
Eastes, R. W.
Martinis, C. R.
Daniell, R. E.
Pedatella, N. M.
Burns, A. G.
McClintock, W.
Goncharenko, L. P.
Coster, A.
Milla, Marco
Wang, W.
Valladares, C. E.
Codrescu, M. V.
dc.subject.none.fl_str_mv Airglow
Total electron content
Thermosphere‐ionosphere dynamics
Equatorial ionization anomaly
topic Airglow
Total electron content
Thermosphere‐ionosphere dynamics
Equatorial ionization anomaly
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 During geomagnetically quiet and solar minimum conditions, spatial variations of the early morning thermosphere‐ionosphere (TI) system are expected to be mainly governed by wave dynamics. To study the postmidnight dynamical coupling, we investigated the early morning equatorial ionization anomaly (EIA) using Global‐scale Observations of the Limb and Disk (GOLD) measurements of OI‐135.6 nm nightglow emission and global navigation satellite system (GNSS)‐based total electron content (TEC) maps. The EIA structures in the OI‐135.6 nm emission over the American landmass resemble, spatially and temporally, those observed in the GNSS‐TEC maps. The early morning EIA (EM‐EIA) crests are well separated in latitude and mostly located over the middle of South America during October–November. In February–April the crests are less separated in latitude and predominantly located over the west coast sector of South America. Whole Atmosphere Community Climate Model with thermosphere and ionosphere eXtension (WACCMX) simulations with constant solar minimum and quiet‐geomagnetic conditions show that EM‐EIA can occur globally and shows properties similar to longitudinal Wave 4 pattern. Thus, we propose that EM‐EIA is driven by dynamical changes associated with the lower atmospheric waves.
publishDate 2020
dc.date.accessioned.none.fl_str_mv 2021-02-16T12:09:25Z
dc.date.available.none.fl_str_mv 2021-02-16T12:09:25Z
dc.date.issued.fl_str_mv 2020-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Laskar, F. I., Eastes, R. W., Martinis, C. R., Daniell, R. E., Pedatella, N. M., Burns, A. G., ... & Codrescu, M. V. (2020). Early morning equatorial ionization anomaly from GOLD observations.==$Journal of Geophysical Research: Space Physics, 125$==(7), e2019JA027487. https://doi.org/10.1029/2019JA027487
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/4917
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1029/2019JA027487
identifier_str_mv Laskar, F. I., Eastes, R. W., Martinis, C. R., Daniell, R. E., Pedatella, N. M., Burns, A. G., ... & Codrescu, M. V. (2020). Early morning equatorial ionization anomaly from GOLD observations.==$Journal of Geophysical Research: Space Physics, 125$==(7), e2019JA027487. https://doi.org/10.1029/2019JA027487
index-oti2018
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/4917
https://doi.org/10.1029/2019JA027487
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 Laskar, F. I.Eastes, R. W.Martinis, C. R.Daniell, R. E.Pedatella, N. M.Burns, A. G.McClintock, W.Goncharenko, L. P.Coster, A.Milla, MarcoWang, W.Valladares, C. E.Codrescu, M. V.2021-02-16T12:09:25Z2021-02-16T12:09:25Z2020-07Laskar, F. I., Eastes, R. W., Martinis, C. R., Daniell, R. E., Pedatella, N. M., Burns, A. G., ... & Codrescu, M. V. (2020). Early morning equatorial ionization anomaly from GOLD observations.==$Journal of Geophysical Research: Space Physics, 125$==(7), e2019JA027487. https://doi.org/10.1029/2019JA027487index-oti2018http://hdl.handle.net/20.500.12816/4917Journal of Geophysical Research: Space Physicshttps://doi.org/10.1029/2019JA027487During geomagnetically quiet and solar minimum conditions, spatial variations of the early morning thermosphere‐ionosphere (TI) system are expected to be mainly governed by wave dynamics. To study the postmidnight dynamical coupling, we investigated the early morning equatorial ionization anomaly (EIA) using Global‐scale Observations of the Limb and Disk (GOLD) measurements of OI‐135.6 nm nightglow emission and global navigation satellite system (GNSS)‐based total electron content (TEC) maps. The EIA structures in the OI‐135.6 nm emission over the American landmass resemble, spatially and temporally, those observed in the GNSS‐TEC maps. The early morning EIA (EM‐EIA) crests are well separated in latitude and mostly located over the middle of South America during October–November. In February–April the crests are less separated in latitude and predominantly located over the west coast sector of South America. Whole Atmosphere Community Climate Model with thermosphere and ionosphere eXtension (WACCMX) simulations with constant solar minimum and quiet‐geomagnetic conditions show that EM‐EIA can occur globally and shows properties similar to longitudinal Wave 4 pattern. 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