Multistatic specular meteor radar network in Peru: system description and initial results
Descripción del Articulo
The mesosphere and lower thermosphere (MLT) region is dominated globally by dynamics at various scales: planetary waves, tides, gravity waves, and stratified turbulence. The latter two can coexist and be significant at horizontal scales less than 500 km, scales that are difficult to measure. This st...
Autores: | , , , , , , , , |
---|---|
Formato: | artículo |
Fecha de Publicación: | 2021 |
Institución: | Instituto Geofísico del Perú |
Repositorio: | IGP-Institucional |
Lenguaje: | inglés |
OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/4922 |
Enlace del recurso: | http://hdl.handle.net/20.500.12816/4922 https://doi.org/10.1029/2020EA001293 |
Nivel de acceso: | acceso abierto |
Materia: | Low latitude mesosphere MLT dynamics MLT horizontal divergence MLT vorticity Multistatic radar observations Vertical velocity https://purl.org/pe-repo/ocde/ford#1.05.01 |
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dc.title.none.fl_str_mv |
Multistatic specular meteor radar network in Peru: system description and initial results |
title |
Multistatic specular meteor radar network in Peru: system description and initial results |
spellingShingle |
Multistatic specular meteor radar network in Peru: system description and initial results Chau, J. L. Low latitude mesosphere MLT dynamics MLT horizontal divergence MLT vorticity Multistatic radar observations Vertical velocity https://purl.org/pe-repo/ocde/ford#1.05.01 |
title_short |
Multistatic specular meteor radar network in Peru: system description and initial results |
title_full |
Multistatic specular meteor radar network in Peru: system description and initial results |
title_fullStr |
Multistatic specular meteor radar network in Peru: system description and initial results |
title_full_unstemmed |
Multistatic specular meteor radar network in Peru: system description and initial results |
title_sort |
Multistatic specular meteor radar network in Peru: system description and initial results |
author |
Chau, J. L. |
author_facet |
Chau, J. L. Urco, J. M. Vierinen, J. Harding, B. J. Clahsen, M. Pfeffer, N. Kuyeng, Karim Milla, Marco Erickson, P. J. |
author_role |
author |
author2 |
Urco, J. M. Vierinen, J. Harding, B. J. Clahsen, M. Pfeffer, N. Kuyeng, Karim Milla, Marco Erickson, P. J. |
author2_role |
author author author author author author author author |
dc.contributor.author.fl_str_mv |
Chau, J. L. Urco, J. M. Vierinen, J. Harding, B. J. Clahsen, M. Pfeffer, N. Kuyeng, Karim Milla, Marco Erickson, P. J. |
dc.subject.none.fl_str_mv |
Low latitude mesosphere MLT dynamics MLT horizontal divergence MLT vorticity Multistatic radar observations Vertical velocity |
topic |
Low latitude mesosphere MLT dynamics MLT horizontal divergence MLT vorticity Multistatic radar observations Vertical velocity https://purl.org/pe-repo/ocde/ford#1.05.01 |
dc.subject.ocde.none.fl_str_mv |
https://purl.org/pe-repo/ocde/ford#1.05.01 |
description |
The mesosphere and lower thermosphere (MLT) region is dominated globally by dynamics at various scales: planetary waves, tides, gravity waves, and stratified turbulence. The latter two can coexist and be significant at horizontal scales less than 500 km, scales that are difficult to measure. This study presents a recently deployed multistatic specular meteor radar system, SIMONe Peru, which can be used to observe these scales. The radars are positioned at and around the Jicamarca Radio Observatory, which is located at the magnetic equator. Besides presenting preliminary results of typically reported large‐scale features, like the dominant diurnal tide at low latitudes, we show results on selected days of spatially and temporally resolved winds obtained with two methods based on: (a) estimation of mean wind and their gradients (gradient method), and (b) an inverse theory with Tikhonov regularization (regularized wind field inversion method). The gradient method allows improved MLT vertical velocities and, for the first time, low‐latitude wind field parameters such as horizontal divergence and relative vorticity. The regularized wind field inversion method allows the estimation of spatial structure within the observed area and has the potential to outperform the gradient method, in particular when more detections are available or when fine adaptive tuning of the regularization factor is done. SIMONe Peru adds important information at low latitudes to currently scarce MLT continuous observing capabilities. Results contribute to studies of the MLT dynamics at different scales inherently connected to lower atmospheric forcing and E‐region dynamo related ionospheric variability. |
publishDate |
2021 |
dc.date.accessioned.none.fl_str_mv |
2021-02-17T13:01:00Z |
dc.date.available.none.fl_str_mv |
2021-02-17T13:01:00Z |
dc.date.issued.fl_str_mv |
2021-01 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
dc.identifier.citation.none.fl_str_mv |
Chau, J. L., Urco, J. M., Vierinen, J., Harding, B. J., Clahsen, M., Pfeffer, N., ... & Erickson, P. J. (2021). Multistatic specular meteor radar network in Peru: system description and initial results.==$Earth and Space Science, 8$==(1), e2020EA001293. https://doi.org/10.1029/2020EA001293 |
dc.identifier.govdoc.none.fl_str_mv |
index-oti2018 |
dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/4922 |
dc.identifier.journal.none.fl_str_mv |
Earth and Space Science |
dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.1029/2020EA001293 |
identifier_str_mv |
Chau, J. L., Urco, J. M., Vierinen, J., Harding, B. J., Clahsen, M., Pfeffer, N., ... & Erickson, P. J. (2021). Multistatic specular meteor radar network in Peru: system description and initial results.==$Earth and Space Science, 8$==(1), e2020EA001293. https://doi.org/10.1029/2020EA001293 index-oti2018 Earth and Space Science |
url |
http://hdl.handle.net/20.500.12816/4922 https://doi.org/10.1029/2020EA001293 |
dc.language.iso.none.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.none.fl_str_mv |
urn:issn:2333-5084 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.uri.none.fl_str_mv |
https://creativecommons.org/licenses/by-nc/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc/4.0/ |
dc.format.none.fl_str_mv |
application/pdf |
dc.coverage.spatial.none.fl_str_mv |
Perú |
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 |
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IGP-Institucional |
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Chau, J. L.Urco, J. M.Vierinen, J.Harding, B. J.Clahsen, M.Pfeffer, N.Kuyeng, KarimMilla, MarcoErickson, P. J.Perú2021-02-17T13:01:00Z2021-02-17T13:01:00Z2021-01Chau, J. L., Urco, J. M., Vierinen, J., Harding, B. J., Clahsen, M., Pfeffer, N., ... & Erickson, P. J. (2021). Multistatic specular meteor radar network in Peru: system description and initial results.==$Earth and Space Science, 8$==(1), e2020EA001293. https://doi.org/10.1029/2020EA001293index-oti2018http://hdl.handle.net/20.500.12816/4922Earth and Space Sciencehttps://doi.org/10.1029/2020EA001293The mesosphere and lower thermosphere (MLT) region is dominated globally by dynamics at various scales: planetary waves, tides, gravity waves, and stratified turbulence. The latter two can coexist and be significant at horizontal scales less than 500 km, scales that are difficult to measure. This study presents a recently deployed multistatic specular meteor radar system, SIMONe Peru, which can be used to observe these scales. The radars are positioned at and around the Jicamarca Radio Observatory, which is located at the magnetic equator. Besides presenting preliminary results of typically reported large‐scale features, like the dominant diurnal tide at low latitudes, we show results on selected days of spatially and temporally resolved winds obtained with two methods based on: (a) estimation of mean wind and their gradients (gradient method), and (b) an inverse theory with Tikhonov regularization (regularized wind field inversion method). The gradient method allows improved MLT vertical velocities and, for the first time, low‐latitude wind field parameters such as horizontal divergence and relative vorticity. The regularized wind field inversion method allows the estimation of spatial structure within the observed area and has the potential to outperform the gradient method, in particular when more detections are available or when fine adaptive tuning of the regularization factor is done. SIMONe Peru adds important information at low latitudes to currently scarce MLT continuous observing capabilities. Results contribute to studies of the MLT dynamics at different scales inherently connected to lower atmospheric forcing and E‐region dynamo related ionospheric variability.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2333-5084info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc/4.0/Low latitude mesosphereMLT dynamicsMLT horizontal divergenceMLT vorticityMultistatic radar observationsVertical velocityhttps://purl.org/pe-repo/ocde/ford#1.05.01Multistatic specular meteor radar network in Peru: system description and initial resultsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALChau_et_al_2021_Earth-and-Space-Science.pdfChau_et_al_2021_Earth-and-Space-Science.pdfapplication/pdf10781494https://repositorio.igp.gob.pe/bitstreams/2df3e6f3-658d-4379-bcb1-9c407ab3e067/download0c7129e7b55095a0fab38bfba5b188a4MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/88dc80f3-2503-43a1-a07e-bc0d97d00c64/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTChau_et_al_2021_Earth-and-Space-Science.pdf.txtChau_et_al_2021_Earth-and-Space-Science.pdf.txtExtracted texttext/plain85404https://repositorio.igp.gob.pe/bitstreams/0b32fa5c-5481-416c-a422-34042fc839e6/download4bd62e103766a8e5118e3949cbc805ceMD53THUMBNAILChau_et_al_2021_Earth-and-Space-Science.pdf.jpgChau_et_al_2021_Earth-and-Space-Science.pdf.jpgIM Thumbnailimage/jpeg48608https://repositorio.igp.gob.pe/bitstreams/597c6b74-755b-435e-af39-7e7f94dc50c0/downloadf2856cb3de4bfa6416110556c742c784MD5420.500.12816/4922oai:repositorio.igp.gob.pe:20.500.12816/49222024-10-12 22:18:28.97https://creativecommons.org/licenses/by-nc/4.0/info:eu-repo/semantics/openAccessopen.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).