A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars

The HF radars of the Super Dual Auroral Radar Network (SuperDARN) provide measurements of the <b><i>E</i></b> × <b><i>B</i></b> drift of ionospheric plasma over extended regions of the high-latitude ionosphere. We have conducted a statistical stu...

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Main Authors: J.-P. Villain, R. André, M. Pinnock, R. A. Greenwald, C. Hanuise
Format: Article
Language:English
Published: Copernicus Publications 2002-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/20/1769/2002/angeo-20-1769-2002.pdf
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author J.-P. Villain
J.-P. Villain
R. André
M. Pinnock
R. A. Greenwald
C. Hanuise
C. Hanuise
author_facet J.-P. Villain
J.-P. Villain
R. André
M. Pinnock
R. A. Greenwald
C. Hanuise
C. Hanuise
author_sort J.-P. Villain
collection DOAJ
description The HF radars of the Super Dual Auroral Radar Network (SuperDARN) provide measurements of the <b><i>E</i></b> × <b><i>B</i></b> drift of ionospheric plasma over extended regions of the high-latitude ionosphere. We have conducted a statistical study of the associated Doppler spectral width of ionospheric F-region echoes. The study has been conducted with all available radars from the Northern Hemisphere for 2 specific periods of time. Period 1 corresponds to the winter months of 1994, while period 2 covers October 1996 to March 1997. The distributions of data points and average spectral width are presented as a function of Magnetic Latitude and Magnetic Local Time. The databases are very consistent and exhibit the same features. The most stringent features are: a region of very high spectral width, collocated with the ionospheric LLBL/cusp/mantle region; an oval shaped region of high spectral width, whose equator-ward boundary matches the poleward limit of the Holzworth and Meng auroral oval. A simulation has been conducted to evaluate the geometrical and instrumental effects on the spectral width. It shows that these effects cannot account for the observed spectral features. It is then concluded that these specific spectral width characteristics are the signature of ionospheric/magnetospheric coupling phenomena.<br><br><b>Key words.</b> Ionosphere (auroral ionosphere; ionosphere-magnetosphere interactions; ionospheric irregularities)
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spelling doaj.art-160fd6ed083940ff9fe92fc3831523122022-12-21T17:57:36ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762002-11-01201769178110.5194/angeo-20-1769-2002A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radarsJ.-P. Villain0J.-P. Villain1R. André2M. Pinnock3R. A. Greenwald4C. Hanuise5C. Hanuise6LPCE/CNRS, 3A Av. de la Recherche Scientifique, 45071 Orléans Cedex, FranceCorrespondence to: J.-P. Villain (jvillain@cnrs-orleans.fr)LPCE/CNRS, 3A Av. de la Recherche Scientifique, 45071 Orléans Cedex, FranceBritish Antarctic Survey, High Cross, Madingley Road, CB3 OET Cambridge, UKThe Johns Hopkins University, Applied Physics Laboratory, Laurel, Maryland, USAnow at LPCE/CNRSLSEET/CNRS, Université de Toulon et du Var, BP 132, 83957 La Garde Cedex, FranceThe HF radars of the Super Dual Auroral Radar Network (SuperDARN) provide measurements of the <b><i>E</i></b> × <b><i>B</i></b> drift of ionospheric plasma over extended regions of the high-latitude ionosphere. We have conducted a statistical study of the associated Doppler spectral width of ionospheric F-region echoes. The study has been conducted with all available radars from the Northern Hemisphere for 2 specific periods of time. Period 1 corresponds to the winter months of 1994, while period 2 covers October 1996 to March 1997. The distributions of data points and average spectral width are presented as a function of Magnetic Latitude and Magnetic Local Time. The databases are very consistent and exhibit the same features. The most stringent features are: a region of very high spectral width, collocated with the ionospheric LLBL/cusp/mantle region; an oval shaped region of high spectral width, whose equator-ward boundary matches the poleward limit of the Holzworth and Meng auroral oval. A simulation has been conducted to evaluate the geometrical and instrumental effects on the spectral width. It shows that these effects cannot account for the observed spectral features. It is then concluded that these specific spectral width characteristics are the signature of ionospheric/magnetospheric coupling phenomena.<br><br><b>Key words.</b> Ionosphere (auroral ionosphere; ionosphere-magnetosphere interactions; ionospheric irregularities)https://www.ann-geophys.net/20/1769/2002/angeo-20-1769-2002.pdf
spellingShingle J.-P. Villain
J.-P. Villain
R. André
M. Pinnock
R. A. Greenwald
C. Hanuise
C. Hanuise
A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars
Annales Geophysicae
title A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars
title_full A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars
title_fullStr A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars
title_full_unstemmed A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars
title_short A Statistical study of the Doppler spectral width of high-latitude ionospheric F-region echoes recorded with SuperDARN coherent HF radars
title_sort statistical study of the doppler spectral width of high latitude ionospheric f region echoes recorded with superdarn coherent hf radars
url https://www.ann-geophys.net/20/1769/2002/angeo-20-1769-2002.pdf
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