Radio-tomographic images of postmidnight equatorial plasma depletions

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For the first time, equatorial plasma depletions (EPDs) have been imaged in the longitude-altitude plane using radiotomography. High-resolution (~10 km) reconstructions of electron density were derived from total electron content (TEC) measurements provided by a receiver array in Peru. TEC data were...

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Detalles Bibliográficos
Autores: Hei, Matthew A., Bernhardt, Paul A., Siefring, Carl L., Wilkens, Matthew R., Huba, Joseph D., Krall, Jonathan F., Valladares, Cesar E., Heelis, Roderick A., Hairston, Marc R., Coley, W. Robin, Chau Chong Shing, Jorge Luis, De la Jara, César
Formato: artículo
Fecha de Publicación:2014
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/1565
Enlace del recurso:http://hdl.handle.net/20.500.12816/1565
https://doi.org/10.1002/2013GL056112
Nivel de acceso:acceso abierto
Materia:Equatorial plasma depletions
Tomography
Equatorial ionosphere
CERTO beacon
C/NOFS satellite
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv Radio-tomographic images of postmidnight equatorial plasma depletions
title Radio-tomographic images of postmidnight equatorial plasma depletions
spellingShingle Radio-tomographic images of postmidnight equatorial plasma depletions
Hei, Matthew A.
Equatorial plasma depletions
Tomography
Equatorial ionosphere
CERTO beacon
C/NOFS satellite
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Radio-tomographic images of postmidnight equatorial plasma depletions
title_full Radio-tomographic images of postmidnight equatorial plasma depletions
title_fullStr Radio-tomographic images of postmidnight equatorial plasma depletions
title_full_unstemmed Radio-tomographic images of postmidnight equatorial plasma depletions
title_sort Radio-tomographic images of postmidnight equatorial plasma depletions
author Hei, Matthew A.
author_facet Hei, Matthew A.
Bernhardt, Paul A.
Siefring, Carl L.
Wilkens, Matthew R.
Huba, Joseph D.
Krall, Jonathan F.
Valladares, Cesar E.
Heelis, Roderick A.
Hairston, Marc R.
Coley, W. Robin
Chau Chong Shing, Jorge Luis
De la Jara, César
author_role author
author2 Bernhardt, Paul A.
Siefring, Carl L.
Wilkens, Matthew R.
Huba, Joseph D.
Krall, Jonathan F.
Valladares, Cesar E.
Heelis, Roderick A.
Hairston, Marc R.
Coley, W. Robin
Chau Chong Shing, Jorge Luis
De la Jara, César
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Hei, Matthew A.
Bernhardt, Paul A.
Siefring, Carl L.
Wilkens, Matthew R.
Huba, Joseph D.
Krall, Jonathan F.
Valladares, Cesar E.
Heelis, Roderick A.
Hairston, Marc R.
Coley, W. Robin
Chau Chong Shing, Jorge Luis
De la Jara, César
dc.subject.none.fl_str_mv Equatorial plasma depletions
Tomography
Equatorial ionosphere
CERTO beacon
C/NOFS satellite
topic Equatorial plasma depletions
Tomography
Equatorial ionosphere
CERTO beacon
C/NOFS satellite
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 For the first time, equatorial plasma depletions (EPDs) have been imaged in the longitude-altitude plane using radiotomography. High-resolution (~10 km) reconstructions of electron density were derived from total electron content (TEC) measurements provided by a receiver array in Peru. TEC data were obtained from VHF/UHF signals transmitted by the C/NOFS CERTO beacon. EPDs generated pre-midnight were observed near dawn. On one night, the bubble densities were highly reduced, 100-1000 km wide, and embedded within a layerlike ionosphere. Three nights later, the EPDs exhibited similar features, but were embedded in a locally uplifted ionosphere. The C/NOFS in-situ instruments detected a dawn depletion where the reconstruction showed lifted EPDs, implying that the postmidnight electric fields raised sections of ionosphere to altitudes where embedded/reactivated fossil-EPDs were detected as dawn depletions. Satellites flying under domelike distortions of the ionosphere may observe these distortions as Broad Plasma Decreases (BPDs).
publishDate 2014
dc.date.accessioned.none.fl_str_mv 2018-06-28T14:32:38Z
dc.date.available.none.fl_str_mv 2018-06-28T14:32:38Z
dc.date.issued.fl_str_mv 2014-01-15
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Hei, M. A., Bernhardt, P. A., Siefring, C. L., Wilkens, M. R., Huba, J. D., Krall, J. F., ... De la Jara, C. (2014). Radio-tomographic images of postmidnight equatorial plasma depletions.==$Geophysical Research Letters, 41$==(1), 13-19. https://doi.org/10.1002/2013GL056112
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/1565
dc.identifier.journal.none.fl_str_mv Geophysical Research Letters
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1002/2013GL056112
identifier_str_mv Hei, M. A., Bernhardt, P. A., Siefring, C. L., Wilkens, M. R., Huba, J. D., Krall, J. F., ... De la Jara, C. (2014). Radio-tomographic images of postmidnight equatorial plasma depletions.==$Geophysical Research Letters, 41$==(1), 13-19. https://doi.org/10.1002/2013GL056112
index-oti2018
Geophysical Research Letters
url http://hdl.handle.net/20.500.12816/1565
https://doi.org/10.1002/2013GL056112
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:0094-8276
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 Hei, Matthew A.Bernhardt, Paul A.Siefring, Carl L.Wilkens, Matthew R.Huba, Joseph D.Krall, Jonathan F.Valladares, Cesar E.Heelis, Roderick A.Hairston, Marc R.Coley, W. RobinChau Chong Shing, Jorge LuisDe la Jara, César2018-06-28T14:32:38Z2018-06-28T14:32:38Z2014-01-15Hei, M. A., Bernhardt, P. A., Siefring, C. L., Wilkens, M. R., Huba, J. D., Krall, J. F., ... De la Jara, C. (2014). Radio-tomographic images of postmidnight equatorial plasma depletions.==$Geophysical Research Letters, 41$==(1), 13-19. https://doi.org/10.1002/2013GL056112index-oti2018http://hdl.handle.net/20.500.12816/1565Geophysical Research Lettershttps://doi.org/10.1002/2013GL056112For the first time, equatorial plasma depletions (EPDs) have been imaged in the longitude-altitude plane using radiotomography. High-resolution (~10 km) reconstructions of electron density were derived from total electron content (TEC) measurements provided by a receiver array in Peru. TEC data were obtained from VHF/UHF signals transmitted by the C/NOFS CERTO beacon. EPDs generated pre-midnight were observed near dawn. On one night, the bubble densities were highly reduced, 100-1000 km wide, and embedded within a layerlike ionosphere. Three nights later, the EPDs exhibited similar features, but were embedded in a locally uplifted ionosphere. The C/NOFS in-situ instruments detected a dawn depletion where the reconstruction showed lifted EPDs, implying that the postmidnight electric fields raised sections of ionosphere to altitudes where embedded/reactivated fossil-EPDs were detected as dawn depletions. Satellites flying under domelike distortions of the ionosphere may observe these distortions as Broad Plasma Decreases (BPDs).Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:0094-8276info:eu-repo/semantics/openAccessEquatorial plasma depletionsTomographyEquatorial ionosphereCERTO beaconC/NOFS satellitehttp://purl.org/pe-repo/ocde/ford#1.05.01Radio-tomographic images of postmidnight equatorial plasma depletionsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALARTHFYF.pdfARTHFYF.pdfapplication/pdf2079999https://repositorio.igp.gob.pe/bitstreams/d0ad4135-b70f-4948-99fe-b21770b8f129/downloadbe763a3946ebd8e9e5029669ef4e1c87MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/e087232b-786d-45ce-ac97-7f34c1a46800/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILARTHFYF.pdf.jpgARTHFYF.pdf.jpgIM Thumbnailimage/jpeg104581https://repositorio.igp.gob.pe/bitstreams/19f61046-9678-4e57-843d-3b69dc8a1aec/download4b0c45d5ed9ce6584370a3a76334469cMD53TEXTARTHFYF.pdf.txtARTHFYF.pdf.txtExtracted texttext/plain38235https://repositorio.igp.gob.pe/bitstreams/a53d0bdd-dc86-46a1-a819-63771cc5719e/download92ddd0ccdbc19c5210c6c81f8ceb27d9MD5420.500.12816/1565oai:repositorio.igp.gob.pe:20.500.12816/15652025-08-13 10:06:32.941open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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