Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/28731
Title: On the spatial distribution of decameter-scale subauroral ionospheric irregularities observed by SuperDARN radars
Authors: de Larquier, S.
Ponomarenko, P.
Ribeiro, A. J.
Ruohoniemi, J. M.
Baker, J. B. H.
Sterne, K. T.
Lester, Mark
First Published: 1-Aug-2013
Publisher: American Geophysical Union
Citation: Journal of Geophysical Research: Space Physics, 2013, 118 (8), pp. 5244-5254
Abstract: The midlatitude Super Dual Auroral Radar Network (SuperDARN) radars regularly observe nighttime low-velocity Sub-Auroral Ionospheric Scatter (SAIS) from decameter-scale ionospheric density irregularities during quiet geomagnetic conditions. To establish the origin of the density irregularities responsible for low-velocity SAIS, it is necessary to distinguish between the effects of high frequency (HF) propagation and irregularity occurrence itself on the observed backscatter distribution. We compare range, azimuth, and elevation data from the Blackstone SuperDARN radar with modeling results from ray tracing coupled with the International Reference Ionosphere assuming a uniform irregularity distribution. The observed and modeled distributions are shown to be very similar. The spatial distribution of backscattering is consistent with the requirement that HF rays propagate nearly perpendicular to the geomagnetic field lines (aspect angle ≤ 1°). For the first time, the irregularities responsible for low-velocity SAIS are determined to extend between 200 and 300 km altitude, validating previous assumptions that low-velocity SAIS is an F-region phenomenon. We find that the limited spatial extent of this category of ionospheric backscatter within SuperDARN radars’ fields-of-view is a consequence of HF propagation effects and the finite vertical extent of the scattering irregularities. We conclude that the density irregularities responsible for low-velocity SAIS are widely distributed horizontally within the midlatitude ionosphere but are confined to the bottom-side F-region.
DOI Link: 10.1002/jgra.50475
ISSN: 2169-9380
eISSN: 2169-9402
Links: http://onlinelibrary.wiley.com/doi/10.1002/jgra.50475/abstract
http://hdl.handle.net/2381/28731
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: © 2013. American Geophysical Union. All Rights Reserved. An edited version of this paper was published by AGU.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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