Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.

Several explanations have been proposed for Naturally Enhanced ion-acoustic Echoes observed at midand high-latitude Incoherent Scatter observatories. A decisive measure for distinguishing between these explanations is whether or not simultaneously observed up- and downshifted enhancement occur simul...

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Main Authors: Grydeland, Tom, Hagfors, T., Trondsen, T.S., Blixt, Erik Mårten, Løvhaug, Unni Pia, La Hoz, Cesar
Format: Article in Journal/Newspaper
Language:English
Published: European Geosciences Union 2004
Subjects:
Online Access:https://hdl.handle.net/10037/546
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author Grydeland, Tom
Hagfors, T.
Trondsen, T.S.
Blixt, Erik Mårten
Løvhaug, Unni Pia
La Hoz, Cesar
author_facet Grydeland, Tom
Hagfors, T.
Trondsen, T.S.
Blixt, Erik Mårten
Løvhaug, Unni Pia
La Hoz, Cesar
author_sort Grydeland, Tom
collection University of Tromsø: Munin Open Research Archive
description Several explanations have been proposed for Naturally Enhanced ion-acoustic Echoes observed at midand high-latitude Incoherent Scatter observatories. A decisive measure for distinguishing between these explanations is whether or not simultaneously observed up- and downshifted enhancement occur simultaneously, or if they are the result of temporal and/or spatial averaging. The EISCAT Svalbard Radar has two antennas in the same radar system, which can be used as an interferometer when pointed parallel. In observations from 17 January 2002, between 06:46:10 and 06:46:30 UT, we used this possibility, in combination with direct sampling of the received signals, to yield measurements of “naturally enhanced ion-acoustic echoes” with sufficiently high resolution to resolve such averaging, if any. For the first time, radar interferometry has been employed to estimate the sizes of coherent structures. The observations were coordinated with an image intensified video camera with a narrow field of view. Together, this forms the initial study on the causal relationships between enhanced echoes and fine structure in the auroral activity on sub-kilometer, sub-second scales. The results confirm that the enhanced echoes originate from very localised regions ( 300m perpendicular to the magnetic field at 500 km altitude) with varying range distribution, and with high time variability ( 200 ms). The corresponding increase in scattering cross section, up to 50 dB above incoherent scattering, eliminates theoretical explanations based on marginal stability. The simultaneously observed up- and down-shifted enhanced shoulders, when caused by sufficiently narrow structures to be detected by the interferometer technique, originate predominantly from the same volume. These results have significant impact on theories attempting to explain the enhancements, in particular it is found that the ion-electron two-stream mechanism favoured by many authors is an unlikely candidate to explain the observations. The video data has helped establish a ...
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 22(2004) pp 1115–1132
https://hdl.handle.net/10037/546
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publisher European Geosciences Union
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spelling ftunivtroemsoe:oai:munin.uit.no:10037/546 2025-04-13T14:18:07+00:00 Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays. Grydeland, Tom Hagfors, T. Trondsen, T.S. Blixt, Erik Mårten Løvhaug, Unni Pia La Hoz, Cesar 2004-04-02 906774 bytes application/pdf https://hdl.handle.net/10037/546 eng eng European Geosciences Union Annales Geophysicae 22(2004) pp 1115–1132 https://hdl.handle.net/10037/546 openAccess auroral ionosphere plasma waves and instabilities radio science (interferometry) VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme akustikk optikk: 434 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 ionosphere Journal article Peer reviewed Tidsskriftartikkel 2004 ftunivtroemsoe 2025-03-14T05:17:55Z Several explanations have been proposed for Naturally Enhanced ion-acoustic Echoes observed at midand high-latitude Incoherent Scatter observatories. A decisive measure for distinguishing between these explanations is whether or not simultaneously observed up- and downshifted enhancement occur simultaneously, or if they are the result of temporal and/or spatial averaging. The EISCAT Svalbard Radar has two antennas in the same radar system, which can be used as an interferometer when pointed parallel. In observations from 17 January 2002, between 06:46:10 and 06:46:30 UT, we used this possibility, in combination with direct sampling of the received signals, to yield measurements of “naturally enhanced ion-acoustic echoes” with sufficiently high resolution to resolve such averaging, if any. For the first time, radar interferometry has been employed to estimate the sizes of coherent structures. The observations were coordinated with an image intensified video camera with a narrow field of view. Together, this forms the initial study on the causal relationships between enhanced echoes and fine structure in the auroral activity on sub-kilometer, sub-second scales. The results confirm that the enhanced echoes originate from very localised regions ( 300m perpendicular to the magnetic field at 500 km altitude) with varying range distribution, and with high time variability ( 200 ms). The corresponding increase in scattering cross section, up to 50 dB above incoherent scattering, eliminates theoretical explanations based on marginal stability. The simultaneously observed up- and down-shifted enhanced shoulders, when caused by sufficiently narrow structures to be detected by the interferometer technique, originate predominantly from the same volume. These results have significant impact on theories attempting to explain the enhancements, in particular it is found that the ion-electron two-stream mechanism favoured by many authors is an unlikely candidate to explain the observations. The video data has helped establish a ... Article in Journal/Newspaper EISCAT Svalbard University of Tromsø: Munin Open Research Archive Svalbard
spellingShingle auroral ionosphere
plasma waves and instabilities
radio science (interferometry)
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
ionosphere
Grydeland, Tom
Hagfors, T.
Trondsen, T.S.
Blixt, Erik Mårten
Løvhaug, Unni Pia
La Hoz, Cesar
Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
title Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
title_full Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
title_fullStr Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
title_full_unstemmed Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
title_short Interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
title_sort interferometric radar observations of filamented structures due to plasma instabilities and their relation to dynamic auroral rays.
topic auroral ionosphere
plasma waves and instabilities
radio science (interferometry)
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
ionosphere
topic_facet auroral ionosphere
plasma waves and instabilities
radio science (interferometry)
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
ionosphere
url https://hdl.handle.net/10037/546