Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm
Descripción del Articulo
There are not too many antennas in the VHF range in the world dedicated to radio astronomy. ST, and specially MST, radars require and have large antenna apertures which could also be used for radio astronomical observations. Definitely, the Jicamarca antenna, the largest in the world (300 m x 300 m)...
Autores: | , |
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Formato: | documento de trabajo |
Fecha de Publicación: | 1995 |
Institución: | Instituto Geofísico del Perú |
Repositorio: | IGP-Institucional |
Lenguaje: | inglés |
OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/592 |
Enlace del recurso: | http://hdl.handle.net/20.500.12816/592 |
Nivel de acceso: | acceso abierto |
Materia: | Shortwave radio Signal processing Astronomy radio Radar http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.03.08 |
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dc.title.none.fl_str_mv |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
title |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
spellingShingle |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm Woodman Pollitt, Ronald Francisco Shortwave radio Signal processing Astronomy radio Radar http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.03.08 |
title_short |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
title_full |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
title_fullStr |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
title_full_unstemmed |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
title_sort |
Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm |
author |
Woodman Pollitt, Ronald Francisco |
author_facet |
Woodman Pollitt, Ronald Francisco Sarango, Martín |
author_role |
author |
author2 |
Sarango, Martín |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Woodman Pollitt, Ronald Francisco Sarango, Martín |
dc.subject.none.fl_str_mv |
Shortwave radio Signal processing Astronomy radio Radar |
topic |
Shortwave radio Signal processing Astronomy radio Radar http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.03.08 |
dc.subject.ocde.none.fl_str_mv |
http://purl.org/pe-repo/ocde/ford#1.05.01 http://purl.org/pe-repo/ocde/ford#1.03.08 |
description |
There are not too many antennas in the VHF range in the world dedicated to radio astronomy. ST, and specially MST, radars require and have large antenna apertures which could also be used for radio astronomical observations. Definitely, the Jicamarca antenna, the largest in the world (300 m x 300 m), has a potential in this field which has not been fully exploited. The present paper was motivated by such application. In addition to the antennas, all radars, do their signal processing using digital equipment, which could also e used for this additional application. However, because of the large processing speed required by radio astronomy, some ingenuity and innovation is required. |
publishDate |
1995 |
dc.date.accessioned.none.fl_str_mv |
2017-12-21T19:41:48Z |
dc.date.available.none.fl_str_mv |
2017-12-21T19:41:48Z |
dc.date.issued.fl_str_mv |
1995 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/workingPaper |
format |
workingPaper |
dc.identifier.citation.none.fl_str_mv |
Woodman, R. F., & Sarango, M. (1995). Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm. |
dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/592 |
identifier_str_mv |
Woodman, R. F., & Sarango, M. (1995). Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm. |
url |
http://hdl.handle.net/20.500.12816/592 |
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/licences/by/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licences/by/4.0/ |
dc.format.none.fl_str_mv |
application/pdf |
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Woodman Pollitt, Ronald FranciscoSarango, Martín2017-12-21T19:41:48Z2017-12-21T19:41:48Z1995Woodman, R. F., & Sarango, M. (1995). Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithm.http://hdl.handle.net/20.500.12816/592There are not too many antennas in the VHF range in the world dedicated to radio astronomy. ST, and specially MST, radars require and have large antenna apertures which could also be used for radio astronomical observations. Definitely, the Jicamarca antenna, the largest in the world (300 m x 300 m), has a potential in this field which has not been fully exploited. The present paper was motivated by such application. In addition to the antennas, all radars, do their signal processing using digital equipment, which could also e used for this additional application. However, because of the large processing speed required by radio astronomy, some ingenuity and innovation is required.IGP, ROJapplication/pdfengEditor no identificadoinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/Shortwave radioSignal processingAstronomy radioRadarhttp://purl.org/pe-repo/ocde/ford#1.05.01http://purl.org/pe-repo/ocde/ford#1.03.08Doing passive radio astronomy with a MST/ST System: a fast crosscorrelation algorithminfo:eu-repo/semantics/workingPaperreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALDoing Passive Radio Astronomy With a MST_ST SYSTEM- A Fast Crosscorrelation Algorithm.pdfapplication/pdf1792480https://repositorio.igp.gob.pe/bitstreams/b3655965-3b6b-455a-ba68-551745247f97/download7d2e1e70d4e9f795cc18a7a18bb8d465MD51LICENSElicense.txttext/plain1748https://repositorio.igp.gob.pe/bitstreams/7bd2bf52-6c5c-4fb9-a638-e5ad066c30e9/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILDoing Passive Radio Astronomy With a MST_ST SYSTEM- A Fast Crosscorrelation Algorithm.pdf.jpgDoing Passive Radio Astronomy With a MST_ST SYSTEM- A Fast Crosscorrelation Algorithm.pdf.jpgIM Thumbnailimage/jpeg92559https://repositorio.igp.gob.pe/bitstreams/3df3a564-cc18-493d-afe9-1c762b209fc8/download07d1caaeb64ca6ea0bbccf4b77859577MD53TEXTDoing Passive Radio Astronomy With a MST_ST SYSTEM- A Fast Crosscorrelation Algorithm.pdf.txtDoing Passive Radio Astronomy With a MST_ST SYSTEM- A Fast Crosscorrelation Algorithm.pdf.txtExtracted texttext/plain4https://repositorio.igp.gob.pe/bitstreams/31d9b26f-8c81-459f-88e5-885ea62f365c/downloadff4c8ff01d544500ea4bfea43e6108c1MD5420.500.12816/592oai:repositorio.igp.gob.pe:20.500.12816/5922024-10-12 22:19:04.625https://creativecommons.org/licences/by/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).