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...
Autores: | , , , , , , , , , , , , |
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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 |
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Instituto Geofísico del Perú |
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IGP |
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IGP |
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IGP-Institucional |
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IGP-Institucional |
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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. Thus, we propose that EM‐EIA is driven by dynamical changes associated with the lower atmospheric waves.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccessAirglowTotal electron contentThermosphere‐ionosphere dynamicsEquatorial ionization anomalyhttp://purl.org/pe-repo/ocde/ford#1.05.01Early morning equatorial ionization anomaly from GOLD observationsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPLICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/344e3394-6f25-44f4-963e-50bfd2ff9818/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTLaskar_et_al_2020_JGR-Space-Physics.pdf.txtLaskar_et_al_2020_JGR-Space-Physics.pdf.txtExtracted texttext/plain44277https://repositorio.igp.gob.pe/bitstreams/ac23107d-9a11-4137-8849-886eabfcfd5a/download5b6eb86f18dd24de8a58826c30ee81e8MD53ORIGINALLaskar_et_al_2020_JGR-Space-Physics.pdfapplication/pdf18540431https://repositorio.igp.gob.pe/bitstreams/2ba50bac-c6aa-472f-bd06-609f41b1be4d/download9792c7db801c54499c4a16771e5f7674MD56THUMBNAILLaskar_et_al_2020_JGR-Space-Physics.pdf.jpgLaskar_et_al_2020_JGR-Space-Physics.pdf.jpgIM Thumbnailimage/jpeg50005https://repositorio.igp.gob.pe/bitstreams/39129aba-35a4-4745-b98b-866176fda98d/download963f07ccc7f5b43a381170653176b9ebMD5520.500.12816/4917oai:repositorio.igp.gob.pe:20.500.12816/49172025-08-21 11:09:33.813open.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).
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).