Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)

Descripción del Articulo

Poster presented at the 2021 CEDAR Virtual Workshop, June 20-25.
Detalles Bibliográficos
Autores: Flores, R., Milla, Marco, Kuyeng, K.
Formato: objeto de conferencia
Fecha de Publicación:2021
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/4968
Enlace del recurso:http://hdl.handle.net/20.500.12816/4968
Nivel de acceso:acceso abierto
Materia:Electron density
Spectra analysis
Remove outliers
https://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.es_ES.fl_str_mv Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
title Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
spellingShingle Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
Flores, R.
Electron density
Spectra analysis
Remove outliers
https://purl.org/pe-repo/ocde/ford#1.05.01
title_short Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
title_full Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
title_fullStr Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
title_full_unstemmed Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
title_sort Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
author Flores, R.
author_facet Flores, R.
Milla, Marco
Kuyeng, K.
author_role author
author2 Milla, Marco
Kuyeng, K.
author2_role author
author
dc.contributor.author.fl_str_mv Flores, R.
Milla, Marco
Kuyeng, K.
dc.subject.es_ES.fl_str_mv Electron density
Spectra analysis
Remove outliers
topic Electron density
Spectra analysis
Remove outliers
https://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.es_ES.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.05.01
description Poster presented at the 2021 CEDAR Virtual Workshop, June 20-25.
publishDate 2021
dc.date.accessioned.none.fl_str_mv 2021-07-09T14:56:27Z
dc.date.available.none.fl_str_mv 2021-07-09T14:56:27Z
dc.date.issued.fl_str_mv 2021-06
dc.type.es_ES.fl_str_mv info:eu-repo/semantics/conferenceObject
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dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/4968
url http://hdl.handle.net/20.500.12816/4968
dc.language.iso.es_ES.fl_str_mv eng
language eng
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eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv Instituto Geofísico del Perú
dc.source.none.fl_str_mv reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
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instname_str Instituto Geofísico del Perú
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spelling Flores, R.Milla, MarcoKuyeng, K.2021-07-09T14:56:27Z2021-07-09T14:56:27Z2021-06http://hdl.handle.net/20.500.12816/4968Poster presented at the 2021 CEDAR Virtual Workshop, June 20-25.At the Geophysical Institute of Peru, specifically on its Jicamarca Radio Observatory (JRO) facility, there are different operation modes to obtain the main parameters of the equatorial ionosphere. One of these modes is the Faraday/Double Pulse which estimates plasma densities and electron/ion temperatures at the F region by pointing the antenna beam off perpendicular to the magnetic field. The data processing for this mode is currently done by using voltage analysis, but in order to obtain better results, spectra analysis has been implemented by using the radar data processing library developed at JRO called Signal Chain. This tool can analyze samples with the same lag and it is also possible to remove the DC clutter from them. Another advantage is that before making the incoherent integration over the spectra, these data can be stored and the outliers from samples with the same frequency can be removed. Comparisons between the different processing programs are shown on this work.application/pdfengInstituto Geofísico del Perúinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/Electron densitySpectra analysisRemove outliershttps://purl.org/pe-repo/ocde/ford#1.05.01Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)info:eu-repo/semantics/conferenceObjectreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALPoster_Flores_et_al_2021.pdfPoster_Flores_et_al_2021.pdfapplication/pdf4155856https://repositorio.igp.gob.pe/bitstreams/f9624ae9-0680-4d8d-80f8-436ef475f62a/download75b91e4b2d8ec29728f159dfc3152cd8MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/d288c79b-d8c8-442c-995c-b0d641ad5cc2/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTPoster_Flores_et_al_2021.pdf.txtPoster_Flores_et_al_2021.pdf.txtExtracted texttext/plain4370https://repositorio.igp.gob.pe/bitstreams/087ffdc1-e9aa-4915-af85-94a3050de021/download781aa35d7cec7ddffba99612bc395c22MD53THUMBNAILPoster_Flores_et_al_2021.pdf.jpgPoster_Flores_et_al_2021.pdf.jpgIM Thumbnailimage/jpeg145006https://repositorio.igp.gob.pe/bitstreams/0561d0d7-e7f5-427a-b0d5-c554ae1dbd64/download02d466e041a479f57e9cff5f384a584aMD5420.500.12816/4968oai:repositorio.igp.gob.pe:20.500.12816/49682021-07-09 15:04:17.784https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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Spectra analysis in Faraday/Double Pulse experiment at Jicamarca Radio Observatory (JRO)
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