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...
Autores: | , |
---|---|
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 |
dc.type.es_ES.fl_str_mv |
info:eu-repo/semantics/conferenceObject |
format |
conferenceObject |
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 |
dc.rights.es_ES.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.uri.es_ES.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.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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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. For transmission we have used four sets of codes, where each code consists of 4 by 4 elements.application/pdfengInstituto Geofísico del Perú, Radio Observatorio de Jicamarcainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/Image processingAntennasStratosphereJicamarca Radio Observatoryhttp://purl.org/pe-repo/ocde/ford#1.05.01http://purl.org/pe-repo/ocde/ford#1.05.00Wide-beam forming using binary phase codinginfo:eu-repo/semantics/conferenceObjectreponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPLICENSElicense.txttext/plain1748https://repositorio.igp.gob.pe/bitstreams/c140fb6c-8a18-4330-a8ef-906c7a34d034/download8a4605be74aa9ea9d79846c1fba20a33MD52TEXTWide-beam forming using binary phase coding.PDF.txtWide-beam forming using binary phase coding.PDF.txtExtracted texttext/plain2https://repositorio.igp.gob.pe/bitstreams/33e93009-5162-48b5-9fc7-d8fb71854ec1/downloade1c06d85ae7b8b032bef47e42e4c08f9MD54Wide-beam_forming_using_binary_phase_coding.pdf.txtWide-beam_forming_using_binary_phase_coding.pdf.txtExtracted texttext/plain1https://repositorio.igp.gob.pe/bitstreams/e57a7871-4252-4231-a4a0-38578f031166/download68b329da9893e34099c7d8ad5cb9c940MD56ORIGINALWide-beam_forming_using_binary_phase_coding.pdfWide-beam_forming_using_binary_phase_coding.pdfapplication/pdf522113https://repositorio.igp.gob.pe/bitstreams/6acf9fc6-269b-4541-8ed9-4d97a0bb5705/download559eb311f2927909e72d4a5329c5b6a0MD55THUMBNAILWide-beam_forming_using_binary_phase_coding.pdf.jpgWide-beam_forming_using_binary_phase_coding.pdf.jpgIM Thumbnailimage/jpeg143793https://repositorio.igp.gob.pe/bitstreams/753711ef-0db3-4212-a1dd-b38669bea9be/download6ea7f6b8cb8ed43505e76e3ff4a08ea3MD5720.500.12816/559oai:repositorio.igp.gob.pe:20.500.12816/5592021-03-10 12:01:46.624https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico del Perudspace-help@myu.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 |
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