Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy

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Instituto Geofísico del Perú (IGP), through its scientific facility at the Jicamarca Radio Observatory (JRO), monitors the upper atmosphere with different instruments: radars, GNSS receivers, magnetometers, among others. Through a National Science Foundation (NSF) MRI award, two Long Wavelength Arra...

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Detalles Bibliográficos
Autores: Estalla, B., Florentino, J., Milla, Marco, Espinoza, J., Kuyeng, K., Scipión, Danny, Rodrigues, F.
Formato: objeto de conferencia
Fecha de Publicación:2025
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/5745
Enlace del recurso:http://hdl.handle.net/20.500.12816/5745
Nivel de acceso:acceso abierto
Materia:Radar receiver
Remote sounding
Ionospheric survey
FPGA
https://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
title Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
spellingShingle Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
Estalla, B.
Radar receiver
Remote sounding
Ionospheric survey
FPGA
https://purl.org/pe-repo/ocde/ford#1.05.01
title_short Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
title_full Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
title_fullStr Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
title_full_unstemmed Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
title_sort Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
author Estalla, B.
author_facet Estalla, B.
Florentino, J.
Milla, Marco
Espinoza, J.
Kuyeng, K.
Scipión, Danny
Rodrigues, F.
author_role author
author2 Florentino, J.
Milla, Marco
Espinoza, J.
Kuyeng, K.
Scipión, Danny
Rodrigues, F.
author2_role author
author
author
author
author
author
dc.contributor.author.fl_str_mv Estalla, B.
Florentino, J.
Milla, Marco
Espinoza, J.
Kuyeng, K.
Scipión, Danny
Rodrigues, F.
dc.subject.none.fl_str_mv Radar receiver
Remote sounding
Ionospheric survey
FPGA
topic Radar receiver
Remote sounding
Ionospheric survey
FPGA
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 Instituto Geofísico del Perú (IGP), through its scientific facility at the Jicamarca Radio Observatory (JRO), monitors the upper atmosphere with different instruments: radars, GNSS receivers, magnetometers, among others. Through a National Science Foundation (NSF) MRI award, two Long Wavelength Array (LWA) receiving stations will be installed at 50 km south (Santa María) and 170 km east (Huancayo) of Jicamarca. Each station is composed of 256 dual-polarization antennas circularly distributed with a diameter of 100 m. In this poster, we present the development of the radio receiver mode for the Long Wavelength Array (LWA). The receiver consists of 16 AMD Zynq UltraScale+ MPSoC ZCU102 devices and 128 ADS5296A ADCs, configured for 12-bit resolution with a sampling rate of 160 MSPS.
publishDate 2025
dc.date.accessioned.none.fl_str_mv 2025-09-11T22:18:11Z
dc.date.available.none.fl_str_mv 2025-09-11T22:18:11Z
dc.date.issued.fl_str_mv 2025-06
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
format conferenceObject
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/5745
url http://hdl.handle.net/20.500.12816/5745
dc.language.iso.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.uri.none.fl_str_mv https://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/4.0/
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv 2025 CEDAR Workshop
publisher.none.fl_str_mv 2025 CEDAR Workshop
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 Estalla, B.Florentino, J.Milla, MarcoEspinoza, J.Kuyeng, K.Scipión, DannyRodrigues, F.2025-09-11T22:18:11Z2025-09-11T22:18:11Z2025-06http://hdl.handle.net/20.500.12816/5745Instituto Geofísico del Perú (IGP), through its scientific facility at the Jicamarca Radio Observatory (JRO), monitors the upper atmosphere with different instruments: radars, GNSS receivers, magnetometers, among others. Through a National Science Foundation (NSF) MRI award, two Long Wavelength Array (LWA) receiving stations will be installed at 50 km south (Santa María) and 170 km east (Huancayo) of Jicamarca. Each station is composed of 256 dual-polarization antennas circularly distributed with a diameter of 100 m. In this poster, we present the development of the radio receiver mode for the Long Wavelength Array (LWA). The receiver consists of 16 AMD Zynq UltraScale+ MPSoC ZCU102 devices and 128 ADS5296A ADCs, configured for 12-bit resolution with a sampling rate of 160 MSPS.application/pdfeng2025 CEDAR Workshopinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/4.0/Radar receiverRemote soundingIonospheric surveyFPGAhttps://purl.org/pe-repo/ocde/ford#1.05.01Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomyinfo:eu-repo/semantics/conferenceObjectreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPLICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/e1845518-590c-4cad-a1ab-689c2783d3d2/downloadbb9bdc0b3349e4284e09149f943790b4MD51ORIGINALEstalla_2025_CEDAR_Workshop.pdfEstalla_2025_CEDAR_Workshop.pdfapplication/pdf1598546https://repositorio.igp.gob.pe/bitstreams/f67ea258-6e22-4f35-a53a-5bc3bead9f38/downloaddae437d1faf279483790eaaccb6444d1MD52TEXTEstalla_2025_CEDAR_Workshop.pdf.txtEstalla_2025_CEDAR_Workshop.pdf.txtExtracted texttext/plain4222https://repositorio.igp.gob.pe/bitstreams/e0bc0392-bfd6-44d5-bc62-36ee3c317e59/download7814b98fb992cb665dc9c99420bdb2ebMD53THUMBNAILEstalla_2025_CEDAR_Workshop.pdf.jpgEstalla_2025_CEDAR_Workshop.pdf.jpgGenerated Thumbnailimage/jpeg108577https://repositorio.igp.gob.pe/bitstreams/c1783bf4-d8e2-4651-98cf-5bdd3a5f8ad7/download1b4ad55f7c84cfb201008aa501ab3436MD5420.500.12816/5745oai:repositorio.igp.gob.pe:20.500.12816/57452025-09-12 12:00:30.036https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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Development of a radio mode for the long wavelength array (LWA) receiving system to study the equatorial aeronomy
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