Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars
International audience 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. T...
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Online Access: | https://hal.science/hal-03382837 https://hal.science/hal-03382837/document https://hal.science/hal-03382837/file/proof_POLAR_100684_last%20%281%29.pdf https://doi.org/10.1016/j.polar.2021.100684 |
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ftutoulouse3hal:oai:HAL:hal-03382837v1 2024-09-15T18:31:26+00:00 Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars Marcucci, Maria Federica Coco, Igino Massetti, Stefano Pignalberi, Alessio Forsythe, Victoriya Pezzopane, Michael Koustov, Alexander Longo, Simona Biondi, David Simeoli, Enrico Consolini, Giuseppe Laurenza, Monica Marchaudon, Aurélie Satta, Andrea Cirioni, Alessandro de Simone, Angelo Olivieri, Angelo Baù, Alessandro Salvati, Alberto Istituto Nazionale di Astrofisica (INAF) Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Roma (INGV) Istituto Nazionale di Geofisica e Vulcanologia University of Saskatchewan Saskatoon, Canada (U of S) National Research Council of Italy Institut de recherche en astrophysique et planétologie (IRAP) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB) 2021-04-20 https://hal.science/hal-03382837 https://hal.science/hal-03382837/document https://hal.science/hal-03382837/file/proof_POLAR_100684_last%20%281%29.pdf https://doi.org/10.1016/j.polar.2021.100684 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/j.polar.2021.100684 hal-03382837 https://hal.science/hal-03382837 https://hal.science/hal-03382837/document https://hal.science/hal-03382837/file/proof_POLAR_100684_last%20%281%29.pdf doi:10.1016/j.polar.2021.100684 info:eu-repo/semantics/OpenAccess ISSN: 1873-9652 Polar Science https://hal.science/hal-03382837 Polar Science, 2021, 28, pp.100684. ⟨10.1016/j.polar.2021.100684⟩ [PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] info:eu-repo/semantics/article Journal articles 2021 ftutoulouse3hal https://doi.org/10.1016/j.polar.2021.100684 2024-06-25T00:11:19Z International audience 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. Article in Journal/Newspaper Polar Science Polar Science Université Toulouse III - Paul Sabatier: HAL-UPS Polar Science 28 100684 |
institution |
Open Polar |
collection |
Université Toulouse III - Paul Sabatier: HAL-UPS |
op_collection_id |
ftutoulouse3hal |
language |
English |
topic |
[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] |
spellingShingle |
[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] Marcucci, Maria Federica Coco, Igino Massetti, Stefano Pignalberi, Alessio Forsythe, Victoriya Pezzopane, Michael Koustov, Alexander Longo, Simona Biondi, David Simeoli, Enrico Consolini, Giuseppe Laurenza, Monica Marchaudon, Aurélie Satta, Andrea Cirioni, Alessandro de Simone, Angelo Olivieri, Angelo Baù, Alessandro Salvati, Alberto Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars |
topic_facet |
[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] |
description |
International audience 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. |
author2 |
Istituto Nazionale di Astrofisica (INAF) Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Roma (INGV) Istituto Nazionale di Geofisica e Vulcanologia University of Saskatchewan Saskatoon, Canada (U of S) National Research Council of Italy Institut de recherche en astrophysique et planétologie (IRAP) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB) |
format |
Article in Journal/Newspaper |
author |
Marcucci, Maria Federica Coco, Igino Massetti, Stefano Pignalberi, Alessio Forsythe, Victoriya Pezzopane, Michael Koustov, Alexander Longo, Simona Biondi, David Simeoli, Enrico Consolini, Giuseppe Laurenza, Monica Marchaudon, Aurélie Satta, Andrea Cirioni, Alessandro de Simone, Angelo Olivieri, Angelo Baù, Alessandro Salvati, Alberto |
author_facet |
Marcucci, Maria Federica Coco, Igino Massetti, Stefano Pignalberi, Alessio Forsythe, Victoriya Pezzopane, Michael Koustov, Alexander Longo, Simona Biondi, David Simeoli, Enrico Consolini, Giuseppe Laurenza, Monica Marchaudon, Aurélie Satta, Andrea Cirioni, Alessandro de Simone, Angelo Olivieri, Angelo Baù, Alessandro Salvati, Alberto |
author_sort |
Marcucci, Maria Federica |
title |
Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars |
title_short |
Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars |
title_full |
Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars |
title_fullStr |
Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars |
title_full_unstemmed |
Echo occurrence in the southern polar ionosphere for the SuperDARN Dome C East and Dome C North radars |
title_sort |
echo occurrence in the southern polar ionosphere for the superdarn dome c east and dome c north radars |
publisher |
HAL CCSD |
publishDate |
2021 |
url |
https://hal.science/hal-03382837 https://hal.science/hal-03382837/document https://hal.science/hal-03382837/file/proof_POLAR_100684_last%20%281%29.pdf https://doi.org/10.1016/j.polar.2021.100684 |
genre |
Polar Science Polar Science |
genre_facet |
Polar Science Polar Science |
op_source |
ISSN: 1873-9652 Polar Science https://hal.science/hal-03382837 Polar Science, 2021, 28, pp.100684. ⟨10.1016/j.polar.2021.100684⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.polar.2021.100684 hal-03382837 https://hal.science/hal-03382837 https://hal.science/hal-03382837/document https://hal.science/hal-03382837/file/proof_POLAR_100684_last%20%281%29.pdf doi:10.1016/j.polar.2021.100684 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1016/j.polar.2021.100684 |
container_title |
Polar Science |
container_volume |
28 |
container_start_page |
100684 |
_version_ |
1810473146006896640 |