VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca

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Range‐time‐intensity (RTI) plots of 50 MHz radar backscatter detected at Jicamarca from the 150‐km region of the equatorial ionosphere exhibit necklace‐shaped multilayered structures first reported by Kudeki and Fawcett (1993, https://doi.org/10.1029/93GL01256). The backscatter layers also exhibit q...

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Detalles Bibliográficos
Autores: Reyes, Pablo M., Kudeki, Erhan, Lehmacher, Gerald A., Chau, Jorge L., Milla, Marco
Formato: artículo
Fecha de Publicación:2020
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/4918
Enlace del recurso:http://hdl.handle.net/20.500.12816/4918
https://doi.org/10.1029/2019JA027535
Nivel de acceso:acceso abierto
Materia:Equatorial ionosphere
150‐km echoes
Radar scattering
Ionospheric sounding
Gravity waves
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
title VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
spellingShingle VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
Reyes, Pablo M.
Equatorial ionosphere
150‐km echoes
Radar scattering
Ionospheric sounding
Gravity waves
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
title_full VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
title_fullStr VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
title_full_unstemmed VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
title_sort VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
author Reyes, Pablo M.
author_facet Reyes, Pablo M.
Kudeki, Erhan
Lehmacher, Gerald A.
Chau, Jorge L.
Milla, Marco
author_role author
author2 Kudeki, Erhan
Lehmacher, Gerald A.
Chau, Jorge L.
Milla, Marco
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Reyes, Pablo M.
Kudeki, Erhan
Lehmacher, Gerald A.
Chau, Jorge L.
Milla, Marco
dc.subject.none.fl_str_mv Equatorial ionosphere
150‐km echoes
Radar scattering
Ionospheric sounding
Gravity waves
topic Equatorial ionosphere
150‐km echoes
Radar scattering
Ionospheric sounding
Gravity waves
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 Range‐time‐intensity (RTI) plots of 50 MHz radar backscatter detected at Jicamarca from the 150‐km region of the equatorial ionosphere exhibit necklace‐shaped multilayered structures first reported by Kudeki and Fawcett (1993, https://doi.org/10.1029/93GL01256). The backscatter layers also exhibit quasi‐periodic intensity fluctuations with periods of about 5–15 min and are separated from adjacent layers by thin and undulating regions of no detectible power returns. A study of the fluctuating backscatter layers and undulating gap regions will be presented using VIPIR ionosonde data taken at the Jicamarca Radio Observatory simultaneously with high‐resolution 50‐MHz radar backscatter data. VIPIR virtual reflection height variations in time are noted to match the RTI gap‐region undulations very closely at selected VIPIR frequencies (or, equivalently, electron densities at reflection heights). This matching enables assigning “true heights” to VIPIR virtual height contour maps, and a joint study of the contour maps with the 50‐MHz radar RTI maps strongly suggests that correlated fluctuations and undulations observed in VIPIR and 50‐MHz radar data are indicative of gravity wave‐induced variations in the 150‐km region ionosphere. Accordingly, a complete explanation of the 150‐km echo phenomenon will need to include gravity wave coupling and forcing effects in the enhancement and suppression processes that can account for the observed fluctuations and gap‐region features of necklace‐shaped 150‐km echo maps.
publishDate 2020
dc.date.accessioned.none.fl_str_mv 2021-02-16T12:41:34Z
dc.date.available.none.fl_str_mv 2021-02-16T12:41:34Z
dc.date.issued.fl_str_mv 2020-08
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Reyes, P. M., Kudeki, E., Lehmacher, G. A., Chau, J. L., & Milla, M. A. (2020). VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca.==$Journal of Geophysical Research: Space Physics, 125$==(8). https://doi.org/10.1029/2019JA027535
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/4918
dc.identifier.journal.none.fl_str_mv Journal of Geophysical Research: Space Physics
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1029/2019JA027535
identifier_str_mv Reyes, P. M., Kudeki, E., Lehmacher, G. A., Chau, J. L., & Milla, M. A. (2020). VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca.==$Journal of Geophysical Research: Space Physics, 125$==(8). https://doi.org/10.1029/2019JA027535
index-oti2018
Journal of Geophysical Research: Space Physics
url http://hdl.handle.net/20.500.12816/4918
https://doi.org/10.1029/2019JA027535
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.coverage.spatial.none.fl_str_mv Jicamarca
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 Reyes, Pablo M.Kudeki, ErhanLehmacher, Gerald A.Chau, Jorge L.Milla, MarcoJicamarca2021-02-16T12:41:34Z2021-02-16T12:41:34Z2020-08Reyes, P. M., Kudeki, E., Lehmacher, G. A., Chau, J. L., & Milla, M. A. (2020). VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca.==$Journal of Geophysical Research: Space Physics, 125$==(8). https://doi.org/10.1029/2019JA027535index-oti2018http://hdl.handle.net/20.500.12816/4918Journal of Geophysical Research: Space Physicshttps://doi.org/10.1029/2019JA027535Range‐time‐intensity (RTI) plots of 50 MHz radar backscatter detected at Jicamarca from the 150‐km region of the equatorial ionosphere exhibit necklace‐shaped multilayered structures first reported by Kudeki and Fawcett (1993, https://doi.org/10.1029/93GL01256). The backscatter layers also exhibit quasi‐periodic intensity fluctuations with periods of about 5–15 min and are separated from adjacent layers by thin and undulating regions of no detectible power returns. A study of the fluctuating backscatter layers and undulating gap regions will be presented using VIPIR ionosonde data taken at the Jicamarca Radio Observatory simultaneously with high‐resolution 50‐MHz radar backscatter data. VIPIR virtual reflection height variations in time are noted to match the RTI gap‐region undulations very closely at selected VIPIR frequencies (or, equivalently, electron densities at reflection heights). This matching enables assigning “true heights” to VIPIR virtual height contour maps, and a joint study of the contour maps with the 50‐MHz radar RTI maps strongly suggests that correlated fluctuations and undulations observed in VIPIR and 50‐MHz radar data are indicative of gravity wave‐induced variations in the 150‐km region ionosphere. Accordingly, a complete explanation of the 150‐km echo phenomenon will need to include gravity wave coupling and forcing effects in the enhancement and suppression processes that can account for the observed fluctuations and gap‐region features of necklace‐shaped 150‐km echo maps.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccessEquatorial ionosphere150‐km echoesRadar scatteringIonospheric soundingGravity waveshttp://purl.org/pe-repo/ocde/ford#1.05.01VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarcainfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPLICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/f47dd238-d1b0-414b-b030-ec49e04d9c65/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTReyes_et_al_2020_JGR-Space-Physics.pdf.txtReyes_et_al_2020_JGR-Space-Physics.pdf.txtExtracted texttext/plain5304https://repositorio.igp.gob.pe/bitstreams/f11b2d8e-1a26-4b0e-8a66-00c7931f0e0f/download9bcb2142e068985ac4cb2bb918e5a26aMD53ORIGINALReyes_et_al_2020_JGR-Space-Physics.pdfapplication/pdf15092383https://repositorio.igp.gob.pe/bitstreams/cc705510-dc4f-4715-9508-f21daaeead96/downloadb6384425731fa877fab17f154ea94aa8MD56THUMBNAILReyes_et_al_2020_JGR-Space-Physics.pdf.jpgReyes_et_al_2020_JGR-Space-Physics.pdf.jpgIM Thumbnailimage/jpeg46193https://repositorio.igp.gob.pe/bitstreams/33c40b57-2f6a-47f6-bab2-1a4714b78640/download26ef5a5e64c657393da197c2c3450e9aMD5520.500.12816/4918oai:repositorio.igp.gob.pe:20.500.12816/49182025-08-19 10:54:19.65open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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