Multi-frequency observations of E-region HF radar aurora

Multi-frequency observations of E-region coherent backscatter from decametre waves reveal that auroral echoes tend to comprise two spectral components superimposed, one at low Doppler shifts, below 250 ms<sup>-1</sup>, and the other Doppler shifted to near the ion-acoustic speed...

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Main Authors: S. E. Milan, M. Lester, N. Sato
Format: Article
Language:English
Published: Copernicus Publications 2003-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/21/761/2003/angeo-21-761-2003.pdf
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spelling doaj-c1ac3d4f37ea4f4f89c4ea44cf34a61d2020-11-24T23:02:46ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762003-03-012176177710.5194/angeo-21-761-2003Multi-frequency observations of E-region HF radar auroraS. E. Milan0M. Lester1N. Sato2Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UKDepartment of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UKNational Institute of Polar Research, Tokyo 173-8515, JapanMulti-frequency observations of E-region coherent backscatter from decametre waves reveal that auroral echoes tend to comprise two spectral components superimposed, one at low Doppler shifts, below 250 ms<sup>-1</sup>, and the other Doppler shifted to near the ion-acoustic speed or above, up to 800 ms<sup>-1</sup>. The low Doppler shift component occurs at all look directions; Doppler shifts near the ion acoustic speed occur when looking at low flow angles along the direction of the electron drift in the electrojet, and Doppler shifts in excess of the ion acoustic speed occur at intermediate flow angles. The latter population appears most commonly at radar frequencies near 10–12 MHz, with its occurrence decreasing dramatically at higher frequencies. The velocity of the high Doppler shift echoes increases with increasing radar frequency, or irregularity wave number <i>k</i>. The velocity of the low Doppler shift population appears to be suppressed significantly below the line-of-sight component of the electron drift. Initial estimates of the altitude from which scatter occurs suggest that the high Doppler shift echoes originate from higher in the E-region than the low Doppler shift echoes, certainly in the eastward electrojet. We discuss these observations with reference to the theories of de/stabilization of two-stream waves by electron density gradients and electrostatic ion cyclotron waves excited by field-parallel electron drifts.<br><br><b>Key words.</b> Ionosphere (ionospheric irregularities)https://www.ann-geophys.net/21/761/2003/angeo-21-761-2003.pdf
collection DOAJ
language English
format Article
sources DOAJ
author S. E. Milan
M. Lester
N. Sato
spellingShingle S. E. Milan
M. Lester
N. Sato
Multi-frequency observations of E-region HF radar aurora
Annales Geophysicae
author_facet S. E. Milan
M. Lester
N. Sato
author_sort S. E. Milan
title Multi-frequency observations of E-region HF radar aurora
title_short Multi-frequency observations of E-region HF radar aurora
title_full Multi-frequency observations of E-region HF radar aurora
title_fullStr Multi-frequency observations of E-region HF radar aurora
title_full_unstemmed Multi-frequency observations of E-region HF radar aurora
title_sort multi-frequency observations of e-region hf radar aurora
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2003-03-01
description Multi-frequency observations of E-region coherent backscatter from decametre waves reveal that auroral echoes tend to comprise two spectral components superimposed, one at low Doppler shifts, below 250 ms<sup>-1</sup>, and the other Doppler shifted to near the ion-acoustic speed or above, up to 800 ms<sup>-1</sup>. The low Doppler shift component occurs at all look directions; Doppler shifts near the ion acoustic speed occur when looking at low flow angles along the direction of the electron drift in the electrojet, and Doppler shifts in excess of the ion acoustic speed occur at intermediate flow angles. The latter population appears most commonly at radar frequencies near 10–12 MHz, with its occurrence decreasing dramatically at higher frequencies. The velocity of the high Doppler shift echoes increases with increasing radar frequency, or irregularity wave number <i>k</i>. The velocity of the low Doppler shift population appears to be suppressed significantly below the line-of-sight component of the electron drift. Initial estimates of the altitude from which scatter occurs suggest that the high Doppler shift echoes originate from higher in the E-region than the low Doppler shift echoes, certainly in the eastward electrojet. We discuss these observations with reference to the theories of de/stabilization of two-stream waves by electron density gradients and electrostatic ion cyclotron waves excited by field-parallel electron drifts.<br><br><b>Key words.</b> Ionosphere (ionospheric irregularities)
url https://www.ann-geophys.net/21/761/2003/angeo-21-761-2003.pdf
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AT mlester multifrequencyobservationsoferegionhfradaraurora
AT nsato multifrequencyobservationsoferegionhfradaraurora
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