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  5. Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars
 
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Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars

Author(s)
Marcucci, Maria Federica  
INAF-IAPS  
Coco, Igino  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia  
Massetti, Stefano  
INAF-IAPS  
Pignalberi, Alessio  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia  
Forsythe, Victoriya  
ASTRA, LLC, Louisville, CO, USA  
Pezzopane, Michael  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia  
Koustov, Alexander  
ISAS-Univ. of Saskatchewan,Saskatoon, Canada  
Longo, Simona  
CNR-DTA  
Biondi, David  
INAF-IAPS  
Simeoli, Enrico  
CNR-ICT  
Consolini, Giuseppe  
INAF-IAPS  
Laurenza, Monica  
INAF-IAPS  
Marchaudon, Aurélie  
IRAP, CNRS, Toulouse University, CNES, Toulouse, France  
Satta, Andrea Ercole  
CNR-IAS  
Cirioni, Alessandro  
CNR-DTA  
De Simone, Angelo  
CNR-ISMN  
Olivieri, Angelo  
CNR-ICT  
Baù, Alessandro  
University of Milano Bicocca  
Salvati, Alberto  
CNR-ICT  
Language
English
Obiettivo Specifico
2A. Fisica dell'alta atmosfera
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Polar science  
Issue/vol(year)
/28 (2021)
ISSN
1873-9652
Publisher
Elsevier
Pages (printed)
100684
Date Issued
2021
DOI
10.1016/j.polar.2021.100684
URI
https://www.earth-prints.org/handle/2122/14774
Abstract
In this paper, echo occurrence rates for the Dome C East (DCE) and the new Dome C North (DCN) radars are
studied. We report the ionospheric and ground scatter echo occurrence rates for selected periods around
equinoxes and solstices in the final part of the solar cycle XXIV. The occurrence maps built in Altitude Adjusted
Corrected Geomagnetic latitude and Magnetic Local Time coordinates show peculiar patterns highly
variable with season. The comparisons of the radar observations with the International Reference Ionosphere
model electron density and with ray tracing simulations allow us to explain the major features of observed
patterns in terms of electron density variations. The study shows the great potential of the DCE and
DCN radar combination to the Super Dual Auroral Radar Network (SuperDARN) convection mapping in
terms of monitoring key regions of the high-latitude ionosphere critical for understanding of the magnetospheric
dynamics.
Type
article
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