Multistatic specular meteor radar network in Peru: system description and initial results

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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...

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Detalles Bibliográficos
Autores: Chau, J. L., Urco, J. M., Vierinen, J., Harding, B. J., Clahsen, M., Pfeffer, N., Kuyeng, Karim, Milla, Marco, Erickson, P. J.
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
collection IGP-Institucional
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spelling 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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