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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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 |
work_keys_str_mv |
AT randre turbulencecharacteristicsinsideionosphericsmallscaleexpandingstructuresobservedwithsuperdarnhfradars AT chanuise turbulencecharacteristicsinsideionosphericsmallscaleexpandingstructuresobservedwithsuperdarnhfradars AT jpvillain turbulencecharacteristicsinsideionosphericsmallscaleexpandingstructuresobservedwithsuperdarnhfradars AT vkrasnoselskikh turbulencecharacteristicsinsideionosphericsmallscaleexpandingstructuresobservedwithsuperdarnhfradars |
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