Wide-beam forming using binary phase coding

Descripción del Articulo

In imaging work, it is desirable to have the transmitting beam width matched to the receiving one. One possibility to do this at Jicamarca, when single receiving modules are employed, is using one antenna module as the transmitting array (the whole Jicamarca array consists of 8 by 8 modules). Howeve...

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Detalles Bibliográficos
Autores: Woodman Pollitt, Ronald Francisco, Chau Chong Shing, Jorge Luis
Formato: objeto de conferencia
Fecha de Publicación:2000
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/559
Enlace del recurso:http://hdl.handle.net/20.500.12816/559
Nivel de acceso:acceso abierto
Materia:Image processing
Antennas
Stratosphere
Jicamarca Radio Observatory
http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
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dc.title.es_ES.fl_str_mv Wide-beam forming using binary phase coding
title Wide-beam forming using binary phase coding
spellingShingle Wide-beam forming using binary phase coding
Woodman Pollitt, Ronald Francisco
Image processing
Antennas
Stratosphere
Jicamarca Radio Observatory
http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
title_short Wide-beam forming using binary phase coding
title_full Wide-beam forming using binary phase coding
title_fullStr Wide-beam forming using binary phase coding
title_full_unstemmed Wide-beam forming using binary phase coding
title_sort Wide-beam forming using binary phase coding
author Woodman Pollitt, Ronald Francisco
author_facet Woodman Pollitt, Ronald Francisco
Chau Chong Shing, Jorge Luis
author_role author
author2 Chau Chong Shing, Jorge Luis
author2_role author
dc.contributor.author.fl_str_mv Woodman Pollitt, Ronald Francisco
Chau Chong Shing, Jorge Luis
dc.subject.es_ES.fl_str_mv Image processing
Antennas
Stratosphere
Jicamarca Radio Observatory
topic Image processing
Antennas
Stratosphere
Jicamarca Radio Observatory
http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
dc.subject.ocde.es_ES.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
http://purl.org/pe-repo/ocde/ford#1.05.00
description In imaging work, it is desirable to have the transmitting beam width matched to the receiving one. One possibility to do this at Jicamarca, when single receiving modules are employed, is using one antenna module as the transmitting array (the whole Jicamarca array consists of 8 by 8 modules). However, with this solution one cannot transmit the high peak power available at Jicamarca (~2 MW). A second solution, where high transmission power is possible, consist on transmitting with ali the antenna modules, but using 4 different sets ofbinary cedes (0 or 180 phase delays), i.e., a two-dimensional complementary phase code. After the decoding process, the information obtained is equivalent to what one would obtain if the high power were transmitted on a single antenna module. The wide beam information is synthesized by adding the second-order statistics obtained with each set of codes. We have tested this idea at Jicamarca to get three-dimensional images of the tropopause and lower stratosphere. For transmission we have used four sets of codes, where each code consists of 4 by 4 elements.
publishDate 2000
dc.date.accessioned.none.fl_str_mv 2016-11-08T00:56:50Z
2017-12-21T19:41:45Z
dc.date.available.none.fl_str_mv 2016-11-08T00:56:50Z
2017-12-21T19:41:45Z
dc.date.issued.fl_str_mv 2000
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dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/559
url http://hdl.handle.net/20.500.12816/559
dc.language.iso.es_ES.fl_str_mv eng
language eng
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dc.format.es_ES.fl_str_mv application/pdf
dc.publisher.es_ES.fl_str_mv Instituto Geofísico del Perú, Radio Observatorio de Jicamarca
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spelling Woodman Pollitt, Ronald FranciscoChau Chong Shing, Jorge Luis2016-11-08T00:56:50Z2017-12-21T19:41:45Z2016-11-08T00:56:50Z2017-12-21T19:41:45Z2000http://hdl.handle.net/20.500.12816/559In imaging work, it is desirable to have the transmitting beam width matched to the receiving one. One possibility to do this at Jicamarca, when single receiving modules are employed, is using one antenna module as the transmitting array (the whole Jicamarca array consists of 8 by 8 modules). However, with this solution one cannot transmit the high peak power available at Jicamarca (~2 MW). A second solution, where high transmission power is possible, consist on transmitting with ali the antenna modules, but using 4 different sets ofbinary cedes (0 or 180 phase delays), i.e., a two-dimensional complementary phase code. After the decoding process, the information obtained is equivalent to what one would obtain if the high power were transmitted on a single antenna module. The wide beam information is synthesized by adding the second-order statistics obtained with each set of codes. We have tested this idea at Jicamarca to get three-dimensional images of the tropopause and lower stratosphere. 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