Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles
Data collected by the CUTLASS Finland HF radar are used to illustrate the significant difference between the cosine component of the plasma convection in the F-region and the Doppler velocity of the E-region coherent echoes observed at large flow angles. We show that the E-region velocity is ~5...
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doaj-da45dbd05f2040ef9dceb097e18264172020-11-24T21:30:08ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-04-01221177118510.5194/angeo-22-1177-2004Simultaneous HF measurements of E- and F-region Doppler velocities at large flow anglesR. A. Makarevitch0F. Honary1A. V. Koustov2Department of Communication Systems, Lancaster University, Lancaster, LA1 4YR, UKDepartment of Communication Systems, Lancaster University, Lancaster, LA1 4YR, UKInstitute of Space and Atmospheric Sciences, University of Saskatchewan, 116 Science Place, Saskatoon, SK, S7N 5E2, CanadaData collected by the CUTLASS Finland HF radar are used to illustrate the significant difference between the cosine component of the plasma convection in the F-region and the Doppler velocity of the E-region coherent echoes observed at large flow angles. We show that the E-region velocity is ~5 times smaller in magnitude and rotated by ~30° clockwise with respect to convection in the F-region. Also, measurements at flow angles larger than 90° exhibit a completely new feature: Doppler velocity increase with the expected aspect angle and spatial anticorrelation with the backscatter power. By considering DMSP drift-meter measurements we argue that the difference between F- and E-region velocities cannot be interpreted in terms of the convection change with latitude. The observed features in the velocity of the E-region echoes can be explained by taking into account the ion drift contribution to the irregularity phase velocity as predicted by the linear fluid theory.<br><br> <b>Key words.</b> Ionosphere (auroral ionosphere; ionospheric irregularities; plasma convection)https://www.ann-geophys.net/22/1177/2004/angeo-22-1177-2004.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
R. A. Makarevitch F. Honary A. V. Koustov |
spellingShingle |
R. A. Makarevitch F. Honary A. V. Koustov Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles Annales Geophysicae |
author_facet |
R. A. Makarevitch F. Honary A. V. Koustov |
author_sort |
R. A. Makarevitch |
title |
Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles |
title_short |
Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles |
title_full |
Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles |
title_fullStr |
Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles |
title_full_unstemmed |
Simultaneous HF measurements of E- and F-region Doppler velocities at large flow angles |
title_sort |
simultaneous hf measurements of e- and f-region doppler velocities at large flow angles |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2004-04-01 |
description |
Data collected by the CUTLASS Finland HF radar are used to
illustrate the significant difference between the cosine component
of the plasma convection in the F-region and the Doppler velocity
of the E-region coherent echoes observed at large flow angles. We
show that the E-region velocity is ~5 times smaller in
magnitude and rotated by ~30° clockwise with respect to
convection in the F-region. Also, measurements at flow angles
larger than 90° exhibit a completely new feature: Doppler
velocity increase with the expected aspect angle and spatial
anticorrelation with the backscatter power. By considering DMSP
drift-meter measurements we argue that the difference between
F- and E-region velocities cannot be interpreted in terms of the
convection change with latitude. The observed features in the
velocity of the E-region echoes can be explained by taking into
account the ion drift contribution to the irregularity phase
velocity as predicted by the linear fluid theory.<br><br>
<b>Key words.</b> Ionosphere (auroral ionosphere; ionospheric irregularities;
plasma convection) |
url |
https://www.ann-geophys.net/22/1177/2004/angeo-22-1177-2004.pdf |
work_keys_str_mv |
AT ramakarevitch simultaneoushfmeasurementsofeandfregiondopplervelocitiesatlargeflowangles AT fhonary simultaneoushfmeasurementsofeandfregiondopplervelocitiesatlargeflowangles AT avkoustov simultaneoushfmeasurementsofeandfregiondopplervelocitiesatlargeflowangles |
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1725963738855505920 |