Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars

Unusual structures characterized by a very high-velocity divergence have been observed in the high-latitude F-region with SuperDARN radars (André et al., 2000). These structures have been interpreted as due to local demagnetization of the plasma in the ionospheric F-region, during very speci...

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Main Authors: R. André, C. Hanuise, J.-P. Villain, V. Krasnoselskikh
Format: Article
Language:English
Published: Copernicus Publications 2003-08-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/21/1839/2003/angeo-21-1839-2003.pdf
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spelling doaj-1934aff344684c22849c2b2afb48c3ec2020-11-25T00:03:47ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762003-08-01211839184510.5194/angeo-21-1839-2003Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radarsR. André0C. Hanuise1J.-P. Villain2V. Krasnoselskikh3LPCE/CNRS, 3A Av. de la Recherche Scientifique, 45071 Orléans Cedex, FranceLPCE/CNRS, 3A Av. de la Recherche Scientifique, 45071 Orléans Cedex, FranceLPCE/CNRS, 3A Av. de la Recherche Scientifique, 45071 Orléans Cedex, FranceLPCE/CNRS, 3A Av. de la Recherche Scientifique, 45071 Orléans Cedex, FranceUnusual structures characterized by a very high-velocity divergence have been observed in the high-latitude F-region with SuperDARN radars (André et al., 2000). These structures have been interpreted as due to local demagnetization of the plasma in the ionospheric F-region, during very specific geophysical conditions. In this study, the collective wave scattering theory is used to characterize the decameter-scale turbulence (<font face="Symbol">l</font> approx 15 m) inside the structures. The distribution function of the diffusion coefficient is modified when the structures are generated, suggesting that two regimes of turbulence coexist. A temporal analysis decorrelates the two regimes and gives access to the dynamics associated with the structures. It is shown that a high turbulent regime precedes the plasma demagnetization and should be related to an energy deposition. Then a second regime appears when the plasma is demagnetized and disappears simultaneously with the structures. This study is the first application of the collective wave scattering theory to a specific geophysical event.<br><br><b>Key words. </b>Ionosphere (auroral ionosphere; ionospheric irregularities) – Space plasma physics (turbulence)https://www.ann-geophys.net/21/1839/2003/angeo-21-1839-2003.pdf
collection DOAJ
language English
format Article
sources DOAJ
author R. André
C. Hanuise
J.-P. Villain
V. Krasnoselskikh
spellingShingle R. André
C. Hanuise
J.-P. Villain
V. Krasnoselskikh
Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars
Annales Geophysicae
author_facet R. André
C. Hanuise
J.-P. Villain
V. Krasnoselskikh
author_sort R. André
title Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars
title_short Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars
title_full Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars
title_fullStr Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars
title_full_unstemmed Turbulence characteristics inside ionospheric small-scale expanding structures observed with SuperDARN HF radars
title_sort turbulence characteristics inside ionospheric small-scale expanding structures observed with superdarn hf radars
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2003-08-01
description Unusual structures characterized by a very high-velocity divergence have been observed in the high-latitude F-region with SuperDARN radars (André et al., 2000). These structures have been interpreted as due to local demagnetization of the plasma in the ionospheric F-region, during very specific geophysical conditions. In this study, the collective wave scattering theory is used to characterize the decameter-scale turbulence (<font face="Symbol">l</font> approx 15 m) inside the structures. The distribution function of the diffusion coefficient is modified when the structures are generated, suggesting that two regimes of turbulence coexist. A temporal analysis decorrelates the two regimes and gives access to the dynamics associated with the structures. It is shown that a high turbulent regime precedes the plasma demagnetization and should be related to an energy deposition. Then a second regime appears when the plasma is demagnetized and disappears simultaneously with the structures. This study is the first application of the collective wave scattering theory to a specific geophysical event.<br><br><b>Key words. </b>Ionosphere (auroral ionosphere; ionospheric irregularities) – Space plasma physics (turbulence)
url https://www.ann-geophys.net/21/1839/2003/angeo-21-1839-2003.pdf
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