An imaging interferometry capability for the EISCAT Svalbard Radar

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Interferometric imaging (aperture synthesis imaging) is a technique used by radio astronomers to achieve angular resolution that far surpasses what is possible with a single large aperture. A similar technique has been used for radar imaging studies of equatorial ionospheric phenomena at the Jicamar...

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Detalles Bibliográficos
Autores: Grydeland, Tom, Chau Chong Shing, Jorge Luis, La Hoz, C., Brekke, A.
Formato: artículo
Fecha de Publicación:2005
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/1874
Enlace del recurso:http://hdl.handle.net/20.500.12816/1874
https://doi.org/10.5194/angeo-23-221-2005
Nivel de acceso:acceso abierto
Materia:Ionosphere
Interferometry
Space plasma physics
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv An imaging interferometry capability for the EISCAT Svalbard Radar
title An imaging interferometry capability for the EISCAT Svalbard Radar
spellingShingle An imaging interferometry capability for the EISCAT Svalbard Radar
Grydeland, Tom
Ionosphere
Interferometry
Space plasma physics
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short An imaging interferometry capability for the EISCAT Svalbard Radar
title_full An imaging interferometry capability for the EISCAT Svalbard Radar
title_fullStr An imaging interferometry capability for the EISCAT Svalbard Radar
title_full_unstemmed An imaging interferometry capability for the EISCAT Svalbard Radar
title_sort An imaging interferometry capability for the EISCAT Svalbard Radar
author Grydeland, Tom
author_facet Grydeland, Tom
Chau Chong Shing, Jorge Luis
La Hoz, C.
Brekke, A.
author_role author
author2 Chau Chong Shing, Jorge Luis
La Hoz, C.
Brekke, A.
author2_role author
author
author
dc.contributor.author.fl_str_mv Grydeland, Tom
Chau Chong Shing, Jorge Luis
La Hoz, C.
Brekke, A.
dc.subject.none.fl_str_mv Ionosphere
Interferometry
Space plasma physics
topic Ionosphere
Interferometry
Space plasma physics
http://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.none.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
description Interferometric imaging (aperture synthesis imaging) is a technique used by radio astronomers to achieve angular resolution that far surpasses what is possible with a single large aperture. A similar technique has been used for radar imaging studies of equatorial ionospheric phenomena at the Jicamarca Radio Observatory. We present plans for adding an interferometric imaging capability to the EISCAT Svalbard Radar (ESR), a capability which will contribute significantly to several areas of active research, including naturally and artificially enhanced ion-acoustic echoes and their detailed relation in space and time to optical phenomena, polar mesospheric summer echoes (PMSE), and meteor studies. Interferometry using the two antennas of the ESR has demonstra ted the existence of extremely narrow, field-aligned scattering structures, but having only a single baseline is a severe limitation for such studies. Building additional IS-class antennas at the ESR is not a trivial task. However, the very high scattering levels in enhanced ion-acoustic echoes and PMSE means that a passive receiver antenna of more modest gain should still be capable of detecting these echoes. In this paper we pre sent simulations of what an imaging interferometer will be capable of observing for different antenna configurations and brightness distributions, under ideal conditions, using two different image inversion algorithms. We also discuss different antenna and receiver technologies.
publishDate 2005
dc.date.accessioned.none.fl_str_mv 2018-07-16T14:32:17Z
dc.date.available.none.fl_str_mv 2018-07-16T14:32:17Z
dc.date.issued.fl_str_mv 2005-01-31
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dc.identifier.citation.none.fl_str_mv Grydeland, T., Chau, J. L., La Hoz, C., & Brekke, A. (2005). An imaging interferometry capability for the EISCAT Svalbard Radar.==$Annales Geophysicae, 23$==(1), 221-230. https://doi.org/10.5194/angeo-23-221-2005
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/1874
dc.identifier.journal.none.fl_str_mv Annales Geophysicae
dc.identifier.doi.none.fl_str_mv https://doi.org/10.5194/angeo-23-221-2005
identifier_str_mv Grydeland, T., Chau, J. L., La Hoz, C., & Brekke, A. (2005). An imaging interferometry capability for the EISCAT Svalbard Radar.==$Annales Geophysicae, 23$==(1), 221-230. https://doi.org/10.5194/angeo-23-221-2005
index-oti2018
Annales Geophysicae
url http://hdl.handle.net/20.500.12816/1874
https://doi.org/10.5194/angeo-23-221-2005
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:0992-7689
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eu_rights_str_mv openAccess
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dc.publisher.none.fl_str_mv European Geosciences Union (EGU)
publisher.none.fl_str_mv European Geosciences Union (EGU)
dc.source.none.fl_str_mv reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
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institution IGP
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collection IGP-Institucional
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spelling Grydeland, TomChau Chong Shing, Jorge LuisLa Hoz, C.Brekke, A.2018-07-16T14:32:17Z2018-07-16T14:32:17Z2005-01-31Grydeland, T., Chau, J. L., La Hoz, C., & Brekke, A. (2005). An imaging interferometry capability for the EISCAT Svalbard Radar.==$Annales Geophysicae, 23$==(1), 221-230. https://doi.org/10.5194/angeo-23-221-2005index-oti2018http://hdl.handle.net/20.500.12816/1874Annales Geophysicaehttps://doi.org/10.5194/angeo-23-221-2005Interferometric imaging (aperture synthesis imaging) is a technique used by radio astronomers to achieve angular resolution that far surpasses what is possible with a single large aperture. A similar technique has been used for radar imaging studies of equatorial ionospheric phenomena at the Jicamarca Radio Observatory. We present plans for adding an interferometric imaging capability to the EISCAT Svalbard Radar (ESR), a capability which will contribute significantly to several areas of active research, including naturally and artificially enhanced ion-acoustic echoes and their detailed relation in space and time to optical phenomena, polar mesospheric summer echoes (PMSE), and meteor studies. Interferometry using the two antennas of the ESR has demonstra ted the existence of extremely narrow, field-aligned scattering structures, but having only a single baseline is a severe limitation for such studies. Building additional IS-class antennas at the ESR is not a trivial task. However, the very high scattering levels in enhanced ion-acoustic echoes and PMSE means that a passive receiver antenna of more modest gain should still be capable of detecting these echoes. 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