Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly

The South Atlantic Anomaly (SAA) is a region where the geomagnetic field is significantly lower than that of the surrounding area. On the basis of the models of CHAOS-7.8, Mass Spectrometer Incoherent Scatter Model (NRLMSISE-00), and International Reference Ionosphere 2016 (IRI-2016), we theoretical...

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Main Authors: SiQi Yi, XiaoJun Xu, ZiLu Zhou, Qing Chang, Xing Wang, Lei Luo, PeiShan He, Hui Li
Format: Article
Language:English
Published: Science Press 2023-01-01
Series:Earth and Planetary Physics
Subjects:
Online Access:http://www.eppcgs.org/article/doi/10.26464/epp2023015?pageType=en
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author SiQi Yi
XiaoJun Xu
ZiLu Zhou
Qing Chang
Xing Wang
Lei Luo
PeiShan He
Hui Li
author_facet SiQi Yi
XiaoJun Xu
ZiLu Zhou
Qing Chang
Xing Wang
Lei Luo
PeiShan He
Hui Li
author_sort SiQi Yi
collection DOAJ
description The South Atlantic Anomaly (SAA) is a region where the geomagnetic field is significantly lower than that of the surrounding area. On the basis of the models of CHAOS-7.8, Mass Spectrometer Incoherent Scatter Model (NRLMSISE-00), and International Reference Ionosphere 2016 (IRI-2016), we theoretically investigated the lower and upper boundaries of the ionospheric dynamo region inside the SAA. In the ionospheric dynamo region, electrons are coupled with magnetic field lines, whereas ions are decoupled from magnetic field lines. Our results showed that the ionospheric dynamo region inside the SAA is higher and larger than that outside the SAA. We also studied the boundary variations of the dynamo region inside the SAA depending on the seasons and solar activities. We found that the dynamo region inside the SAA is the highest and largest in the summer of the southern hemisphere at solar maximum. The larger and higher altitude range of the ionospheric dynamo region in the SAA can contribute to the stronger ionospheric currents in this region.
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spelling doaj.art-f4b19cc55b6c4742b0250744430095f42023-01-05T06:35:25ZengScience PressEarth and Planetary Physics2096-39552023-01-0171849210.26464/epp202301510-yisiqi-xuxiaojun-FTheoretical study of the ionospheric dynamo region inside the South Atlantic AnomalySiQi Yi0XiaoJun Xu1ZiLu Zhou2Qing Chang3Xing Wang4Lei Luo5PeiShan He6Hui Li7State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa Macao 999078, ChinaState Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, ChinaThe South Atlantic Anomaly (SAA) is a region where the geomagnetic field is significantly lower than that of the surrounding area. On the basis of the models of CHAOS-7.8, Mass Spectrometer Incoherent Scatter Model (NRLMSISE-00), and International Reference Ionosphere 2016 (IRI-2016), we theoretically investigated the lower and upper boundaries of the ionospheric dynamo region inside the SAA. In the ionospheric dynamo region, electrons are coupled with magnetic field lines, whereas ions are decoupled from magnetic field lines. Our results showed that the ionospheric dynamo region inside the SAA is higher and larger than that outside the SAA. We also studied the boundary variations of the dynamo region inside the SAA depending on the seasons and solar activities. We found that the dynamo region inside the SAA is the highest and largest in the summer of the southern hemisphere at solar maximum. The larger and higher altitude range of the ionospheric dynamo region in the SAA can contribute to the stronger ionospheric currents in this region.http://www.eppcgs.org/article/doi/10.26464/epp2023015?pageType=ensouth atlantic anomalyionospheric dynamo regionionosphere
spellingShingle SiQi Yi
XiaoJun Xu
ZiLu Zhou
Qing Chang
Xing Wang
Lei Luo
PeiShan He
Hui Li
Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly
Earth and Planetary Physics
south atlantic anomaly
ionospheric dynamo region
ionosphere
title Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly
title_full Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly
title_fullStr Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly
title_full_unstemmed Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly
title_short Theoretical study of the ionospheric dynamo region inside the South Atlantic Anomaly
title_sort theoretical study of the ionospheric dynamo region inside the south atlantic anomaly
topic south atlantic anomaly
ionospheric dynamo region
ionosphere
url http://www.eppcgs.org/article/doi/10.26464/epp2023015?pageType=en
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