An imaging interferometry capability for the EISCAT Svalbard Radar

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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Published in:Annales Geophysicae
Main Authors: Grydeland, T., Chau, J. L., La Hoz, C., Brekke, A.
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2005
Subjects:
Online Access:https://doi.org/10.5194/angeo-23-221-2005
https://noa.gwlb.de/receive/cop_mods_00034411
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00034365/angeo-23-221-2005.pdf
https://angeo.copernicus.org/articles/23/221/2005/angeo-23-221-2005.pdf
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author Grydeland, T.
Chau, J. L.
La Hoz, C.
Brekke, A.
author_facet Grydeland, T.
Chau, J. L.
La Hoz, C.
Brekke, A.
author_sort Grydeland, T.
collection Niedersächsisches Online-Archiv NOA
container_issue 1
container_start_page 221
container_title Annales Geophysicae
container_volume 23
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 demonstrated 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 present 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.
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Svalbard
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op_doi https://doi.org/10.5194/angeo-23-221-2005
op_relation Annales Geophysicae -- http://www.bibliothek.uni-regensburg.de/ezeit/?1458425 -- https://www.ann-geophys.net/ -- https://www.ann-geophys.net/volumes.html -- http://link.springer.com/journal/585 -- 1432-0576
https://doi.org/10.5194/angeo-23-221-2005
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https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00034365/angeo-23-221-2005.pdf
https://angeo.copernicus.org/articles/23/221/2005/angeo-23-221-2005.pdf
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spelling ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00034411 2025-01-16T21:42:04+00:00 An imaging interferometry capability for the EISCAT Svalbard Radar Grydeland, T. Chau, J. L. La Hoz, C. Brekke, A. 2005-01 electronic https://doi.org/10.5194/angeo-23-221-2005 https://noa.gwlb.de/receive/cop_mods_00034411 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00034365/angeo-23-221-2005.pdf https://angeo.copernicus.org/articles/23/221/2005/angeo-23-221-2005.pdf eng eng Copernicus Publications Annales Geophysicae -- http://www.bibliothek.uni-regensburg.de/ezeit/?1458425 -- https://www.ann-geophys.net/ -- https://www.ann-geophys.net/volumes.html -- http://link.springer.com/journal/585 -- 1432-0576 https://doi.org/10.5194/angeo-23-221-2005 https://noa.gwlb.de/receive/cop_mods_00034411 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00034365/angeo-23-221-2005.pdf https://angeo.copernicus.org/articles/23/221/2005/angeo-23-221-2005.pdf uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2005 ftnonlinearchiv https://doi.org/10.5194/angeo-23-221-2005 2022-02-08T22:45:14Z 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 demonstrated 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 present 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. Article in Journal/Newspaper EISCAT Svalbard Niedersächsisches Online-Archiv NOA Svalbard Annales Geophysicae 23 1 221 230
spellingShingle article
Verlagsveröffentlichung
Grydeland, T.
Chau, J. L.
La Hoz, C.
Brekke, A.
An imaging interferometry capability for the EISCAT Svalbard Radar
title 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_short An imaging interferometry capability for the EISCAT Svalbard Radar
title_sort imaging interferometry capability for the eiscat svalbard radar
topic article
Verlagsveröffentlichung
topic_facet article
Verlagsveröffentlichung
url https://doi.org/10.5194/angeo-23-221-2005
https://noa.gwlb.de/receive/cop_mods_00034411
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00034365/angeo-23-221-2005.pdf
https://angeo.copernicus.org/articles/23/221/2005/angeo-23-221-2005.pdf