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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Main Authors: Chau, J.L., Grydeland, Tom, La Hoz, C., Brekke, Asgeir
Format: Article in Journal/Newspaper
Language:English
Published: European Geosciences Union 2005
Subjects:
Online Access:https://hdl.handle.net/10037/548
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author Chau, J.L.
Grydeland, Tom
La Hoz, C.
Brekke, Asgeir
author_facet Chau, J.L.
Grydeland, Tom
La Hoz, C.
Brekke, Asgeir
author_sort Chau, J.L.
collection University of Tromsø: Munin Open Research Archive
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, fieldaligned 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.
format Article in Journal/Newspaper
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
geographic Svalbard
geographic_facet Svalbard
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institution Open Polar
language English
op_collection_id ftunivtroemsoe
op_relation Annales Geophysicae 23(2005), pp 221-230
https://hdl.handle.net/10037/548
op_rights openAccess
publishDate 2005
publisher European Geosciences Union
record_format openpolar
spelling ftunivtroemsoe:oai:munin.uit.no:10037/548 2025-04-13T14:18:06+00:00 An imaging interferometry capability for the EISCAT Svalbard Radar. Chau, J.L. Grydeland, Tom La Hoz, C. Brekke, Asgeir 2005-01-31 334735 bytes application/pdf https://hdl.handle.net/10037/548 eng eng European Geosciences Union Annales Geophysicae 23(2005), pp 221-230 https://hdl.handle.net/10037/548 openAccess ionosphere instruments and techniques radio science (interferometry) space plasma physics VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme akustikk optikk: 434 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 Journal article Peer reviewed Tidsskriftartikkel 2005 ftunivtroemsoe 2025-03-14T05:17:55Z 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, fieldaligned 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 University of Tromsø: Munin Open Research Archive Svalbard
spellingShingle ionosphere
instruments and techniques
radio science (interferometry)
space plasma physics
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
Chau, J.L.
Grydeland, Tom
La Hoz, C.
Brekke, Asgeir
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 ionosphere
instruments and techniques
radio science (interferometry)
space plasma physics
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
topic_facet ionosphere
instruments and techniques
radio science (interferometry)
space plasma physics
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
url https://hdl.handle.net/10037/548