VIPIR and 50 MHz radar studies of gravity wave signatures in 150‐km echoes observed at Jicamarca
Descripción del Articulo
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...
| Autores: | , , , , |
|---|---|
| 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 |
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info:eu-repo/semantics/openAccess |
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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 |
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reponame:IGP-Institucional instname:Instituto Geofísico del Perú instacron:IGP |
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Instituto Geofísico del Perú |
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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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 |
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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).