E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum

According to the study by Mayer and Jakowski (2009), periods of E layer dominated ionosphere (ELDI) are defined as being characterized by vertical electron density profiles having a maximum density at E layer altitudes. In this paper, characteristics of ELDI intervals have been investigated, focusin...

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Published in:Annales Geophysicae
Main Authors: Cai, Hongtao, Li, Fei, Shen, Ge, Zhan, Weijia, Zhou, Kangjun, McCrea, Ian Willian, Ma, Shuying
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-32-1223-2014
https://angeo.copernicus.org/articles/32/1223/2014/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo23680 2023-05-15T16:04:37+02:00 E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum Cai, Hongtao Li, Fei Shen, Ge Zhan, Weijia Zhou, Kangjun McCrea, Ian Willian Ma, Shuying 2018-09-27 application/pdf https://doi.org/10.5194/angeo-32-1223-2014 https://angeo.copernicus.org/articles/32/1223/2014/ eng eng doi:10.5194/angeo-32-1223-2014 https://angeo.copernicus.org/articles/32/1223/2014/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-32-1223-2014 2020-07-20T16:24:54Z According to the study by Mayer and Jakowski (2009), periods of E layer dominated ionosphere (ELDI) are defined as being characterized by vertical electron density profiles having a maximum density at E layer altitudes. In this paper, characteristics of ELDI intervals have been investigated, focusing on their temporal variations, using field-aligned measurements from the EISCAT and ESR radars during the interval 2009–2011. ELDI events were identified using simple but reasonable criteria, in which a minimal duration was required to exclude possible "fake" events induced by random errors in measurements. It was found that ELDIs were observed more often in winter and earlier spring than other seasons, especially in the auroral zone. The occurrence of ELDI intervals peaks around geomagnetic midnight at auroral latitudes, while it reaches a maximum around geomagnetic local noon at the latitude of the ESR. Our results imply that ELDI intervals appear to be a sporadic rather than a regular phenomenon, in disagreement with previous results inferred from radio occultation measurements. The discrepancy between the typical durations of ELDI events observed by the two radars is remarkable, being 30 min on average at Tromsø but about a half of this at Svalbard. During intervals of ELDI, the mean thicknesses of the E layer are quite close at the two sites, as are the values of H m E and the ratio of N m E / N m F 2 . Case studies confirm that either extra E layer ionization or F layer density depletion alone could lead to the presence of ELDIs. Based on a careful check on ELDI intervals of various types, however, we suggest that both of them play a critical role in ELDI formation. Text EISCAT Svalbard Tromsø Copernicus Publications: E-Journals Svalbard Tromsø Annales Geophysicae 32 10 1223 1231
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description According to the study by Mayer and Jakowski (2009), periods of E layer dominated ionosphere (ELDI) are defined as being characterized by vertical electron density profiles having a maximum density at E layer altitudes. In this paper, characteristics of ELDI intervals have been investigated, focusing on their temporal variations, using field-aligned measurements from the EISCAT and ESR radars during the interval 2009–2011. ELDI events were identified using simple but reasonable criteria, in which a minimal duration was required to exclude possible "fake" events induced by random errors in measurements. It was found that ELDIs were observed more often in winter and earlier spring than other seasons, especially in the auroral zone. The occurrence of ELDI intervals peaks around geomagnetic midnight at auroral latitudes, while it reaches a maximum around geomagnetic local noon at the latitude of the ESR. Our results imply that ELDI intervals appear to be a sporadic rather than a regular phenomenon, in disagreement with previous results inferred from radio occultation measurements. The discrepancy between the typical durations of ELDI events observed by the two radars is remarkable, being 30 min on average at Tromsø but about a half of this at Svalbard. During intervals of ELDI, the mean thicknesses of the E layer are quite close at the two sites, as are the values of H m E and the ratio of N m E / N m F 2 . Case studies confirm that either extra E layer ionization or F layer density depletion alone could lead to the presence of ELDIs. Based on a careful check on ELDI intervals of various types, however, we suggest that both of them play a critical role in ELDI formation.
format Text
author Cai, Hongtao
Li, Fei
Shen, Ge
Zhan, Weijia
Zhou, Kangjun
McCrea, Ian Willian
Ma, Shuying
spellingShingle Cai, Hongtao
Li, Fei
Shen, Ge
Zhan, Weijia
Zhou, Kangjun
McCrea, Ian Willian
Ma, Shuying
E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum
author_facet Cai, Hongtao
Li, Fei
Shen, Ge
Zhan, Weijia
Zhou, Kangjun
McCrea, Ian Willian
Ma, Shuying
author_sort Cai, Hongtao
title E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum
title_short E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum
title_full E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum
title_fullStr E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum
title_full_unstemmed E layer dominated ionosphere observed by EISCAT/ESR radars during solar minimum
title_sort e layer dominated ionosphere observed by eiscat/esr radars during solar minimum
publishDate 2018
url https://doi.org/10.5194/angeo-32-1223-2014
https://angeo.copernicus.org/articles/32/1223/2014/
geographic Svalbard
Tromsø
geographic_facet Svalbard
Tromsø
genre EISCAT
Svalbard
Tromsø
genre_facet EISCAT
Svalbard
Tromsø
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-32-1223-2014
https://angeo.copernicus.org/articles/32/1223/2014/
op_doi https://doi.org/10.5194/angeo-32-1223-2014
container_title Annales Geophysicae
container_volume 32
container_issue 10
container_start_page 1223
op_container_end_page 1231
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