Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms

Intense geomagnetic storms offer opportunity to understand ionospheric response to space weather events. Using Total Electron Content (TEC) data from stations along the east African sector, the two most intense storms during the 24th solar cycle, with similarly occurrence season and time were studi...

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Main Authors: S. O. Ikubanni, S. J. Adebiyi, B. O. Adebesin, O. S. Bolaji, B. J. Adekoya, B. W. Joshua, J. O. Adeniyi
Format: Article
Language:English
Published: Nigerian Society of Physical Sciences 2020-11-01
Series:Journal of Nigerian Society of Physical Sciences
Subjects:
Online Access:https://journal.nsps.org.ng/index.php/jnsps/article/view/112
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spelling doaj-360e3c50712844cb8652d5fe004291152020-11-25T04:09:56ZengNigerian Society of Physical SciencesJournal of Nigerian Society of Physical Sciences2714-28172714-47042020-11-012410.46481/jnsps.2020.112Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic stormsS. O. Ikubanni0S. J. Adebiyi1B. O. Adebesin2O. S. Bolaji3B. J. Adekoya4B. W. Joshua5J. O. Adeniyi6Space Weather Group, Landmark University, P.M.B. 1001, Omu-Aran, NigeriaSpace Weather Group, Landmark University, P.M.B. 1001, Omu-Aran, NigeriaSpace Weather Group, Landmark University, P.M.B. 1001, Omu-Aran, NigeriaDepartment of Physics,University of Tansmania, Australia; Department of Physics, University of Lagos, NigeriaDepartment of Physics, Olabisi Onabanjo University, Ago-Iwoye, Ogun StateDepartment of Physics, Kebbi State University, Aleiro, Kebbi StateSpace Weather Group, Landmark University, P.M.B. 1001, Omu-Aran, Nigeria Intense geomagnetic storms offer opportunity to understand ionospheric response to space weather events. Using Total Electron Content (TEC) data from stations along the east African sector, the two most intense storms during the 24th solar cycle, with similarly occurrence season and time were studied. We observe that ionospheric effect during the main phase is not a function of the severity of the storm, whereas the more intense storm shows greater influence on the African ionosphere during the recovery phase. Plasma movement within the equatorial ionization anomaly (EIA) was evident particularly during the recovery phase, especially during the 2015 event. For both storms, the nighttime/early morning ionospheric effect is more pronounced than the daytime effects across all stations.     https://journal.nsps.org.ng/index.php/jnsps/article/view/112Disturbance Electric FieldEquatorial ionosphereGeomagnetic stormsGNSS
collection DOAJ
language English
format Article
sources DOAJ
author S. O. Ikubanni
S. J. Adebiyi
B. O. Adebesin
O. S. Bolaji
B. J. Adekoya
B. W. Joshua
J. O. Adeniyi
spellingShingle S. O. Ikubanni
S. J. Adebiyi
B. O. Adebesin
O. S. Bolaji
B. J. Adekoya
B. W. Joshua
J. O. Adeniyi
Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms
Journal of Nigerian Society of Physical Sciences
Disturbance Electric Field
Equatorial ionosphere
Geomagnetic storms
GNSS
author_facet S. O. Ikubanni
S. J. Adebiyi
B. O. Adebesin
O. S. Bolaji
B. J. Adekoya
B. W. Joshua
J. O. Adeniyi
author_sort S. O. Ikubanni
title Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms
title_short Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms
title_full Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms
title_fullStr Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms
title_full_unstemmed Plasma re-distribution in the African low-latitude ionosphere during intense geomagnetic storms
title_sort plasma re-distribution in the african low-latitude ionosphere during intense geomagnetic storms
publisher Nigerian Society of Physical Sciences
series Journal of Nigerian Society of Physical Sciences
issn 2714-2817
2714-4704
publishDate 2020-11-01
description Intense geomagnetic storms offer opportunity to understand ionospheric response to space weather events. Using Total Electron Content (TEC) data from stations along the east African sector, the two most intense storms during the 24th solar cycle, with similarly occurrence season and time were studied. We observe that ionospheric effect during the main phase is not a function of the severity of the storm, whereas the more intense storm shows greater influence on the African ionosphere during the recovery phase. Plasma movement within the equatorial ionization anomaly (EIA) was evident particularly during the recovery phase, especially during the 2015 event. For both storms, the nighttime/early morning ionospheric effect is more pronounced than the daytime effects across all stations.    
topic Disturbance Electric Field
Equatorial ionosphere
Geomagnetic storms
GNSS
url https://journal.nsps.org.ng/index.php/jnsps/article/view/112
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