Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels

In this paper, we investigate anomalies in total electron content (TEC) from 7 stations of the Africa Geodetic Reference Frame (AFREF) during the initial and recovery stages of the geomagnetic storm of 19 February 2014. Additionally, we study geomagnetic storms under the solar activity ascending per...

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Main Authors: Chukwuma Moses Anoruo, Babatunde Rabiu, Daniel Okoh, Francisca Nneka Okeke, Kingsley Chukwudi Okpala
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-09-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.947473/full
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author Chukwuma Moses Anoruo
Chukwuma Moses Anoruo
Babatunde Rabiu
Daniel Okoh
Francisca Nneka Okeke
Kingsley Chukwudi Okpala
author_facet Chukwuma Moses Anoruo
Chukwuma Moses Anoruo
Babatunde Rabiu
Daniel Okoh
Francisca Nneka Okeke
Kingsley Chukwudi Okpala
author_sort Chukwuma Moses Anoruo
collection DOAJ
description In this paper, we investigate anomalies in total electron content (TEC) from 7 stations of the Africa Geodetic Reference Frame (AFREF) during the initial and recovery stages of the geomagnetic storm of 19 February 2014. Additionally, we study geomagnetic storms under the solar activity ascending period of March 2012 and low solar activity of May 2017 to emphasize scintillation effects, especially during the nighttime. We employ a 15-days median-average sliding window to study the latitudinal patterns of relative TEC (rTEC) and determine the storm ionospheric irregularities using the rate of TEC index (ROTI). The low-latitude stations show larger rTEC variations during the storm than the midlatitude stations. ROTI strength >1 TECU/min is found at low latitude stations during postsunset and <1 TECU/min at mid latitudes during daytime. The results from this study show that rTEC differences between midlatitude stations may be caused by dynamo of the electric field originating from energy input during geomagnetic disturbances. We observed a low latitude significant intensity of ionospheric irregularities and established that low latitude ionospheric irregularities are more pronounced during the storm initial and recovery stages.
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spelling doaj.art-53c784b94ecb4e448f247a156504ca5d2022-12-22T03:45:00ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2022-09-01910.3389/fspas.2022.947473947473Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levelsChukwuma Moses Anoruo0Chukwuma Moses Anoruo1Babatunde Rabiu2Daniel Okoh3Francisca Nneka Okeke4Kingsley Chukwudi Okpala5Department of Physics and Astronomy, University of Nigeria, Nsukka, NigeriaCenter for Atmospheric Research, National Space Research and Development Agency, Anyigba, NigeriaCenter for Atmospheric Research, National Space Research and Development Agency, Anyigba, NigeriaCenter for Atmospheric Research, National Space Research and Development Agency, Anyigba, NigeriaDepartment of Physics and Astronomy, University of Nigeria, Nsukka, NigeriaDepartment of Physics and Astronomy, University of Nigeria, Nsukka, NigeriaIn this paper, we investigate anomalies in total electron content (TEC) from 7 stations of the Africa Geodetic Reference Frame (AFREF) during the initial and recovery stages of the geomagnetic storm of 19 February 2014. Additionally, we study geomagnetic storms under the solar activity ascending period of March 2012 and low solar activity of May 2017 to emphasize scintillation effects, especially during the nighttime. We employ a 15-days median-average sliding window to study the latitudinal patterns of relative TEC (rTEC) and determine the storm ionospheric irregularities using the rate of TEC index (ROTI). The low-latitude stations show larger rTEC variations during the storm than the midlatitude stations. ROTI strength >1 TECU/min is found at low latitude stations during postsunset and <1 TECU/min at mid latitudes during daytime. The results from this study show that rTEC differences between midlatitude stations may be caused by dynamo of the electric field originating from energy input during geomagnetic disturbances. We observed a low latitude significant intensity of ionospheric irregularities and established that low latitude ionospheric irregularities are more pronounced during the storm initial and recovery stages.https://www.frontiersin.org/articles/10.3389/fspas.2022.947473/fullTEC anomalieslow latitude irregularitiesgeomagnetic stormAfrica geodetic reference frameROTI
spellingShingle Chukwuma Moses Anoruo
Chukwuma Moses Anoruo
Babatunde Rabiu
Daniel Okoh
Francisca Nneka Okeke
Kingsley Chukwudi Okpala
Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels
Frontiers in Astronomy and Space Sciences
TEC anomalies
low latitude irregularities
geomagnetic storm
Africa geodetic reference frame
ROTI
title Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels
title_full Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels
title_fullStr Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels
title_full_unstemmed Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels
title_short Irregularities in the African ionosphere associated with total electron content anomalies observed during high solar activity levels
title_sort irregularities in the african ionosphere associated with total electron content anomalies observed during high solar activity levels
topic TEC anomalies
low latitude irregularities
geomagnetic storm
Africa geodetic reference frame
ROTI
url https://www.frontiersin.org/articles/10.3389/fspas.2022.947473/full
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