Responses of the African and American Equatorial Ionization Anomaly (EIA) to 2014 Arctic SSW Events

Aside from the influence of forcing from above on the ionosphere during space weather, forcing from below also have significant influence on the ionosphere. This study investigates responses of the equatorial ionization anomaly (EIA) in the African and American longitudinal sectors to the combined e...

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Bibliographic Details
Published in:Space Weather 2021-11, Vol.19 (11), p.n/a
Main Authors: Idolor, O. R., Akala, A. O., Bolaji, O. S.
Format: Article
Language:English
Subjects:
Electric field strength
Electrodynamics
Equatorial ionization anomaly
Geomagnetic storms
Geomagnetism
Ionization
Ionosphere
Ionospheric irregularities
Irregularities
Latitude
Magnetic storms
Mean winds
Northern Hemisphere
Polar environments
reverse fountain effect
Skewed distributions
Space weather
Storms
Stratospheric warming
sudden stratospheric warming
vertical drift
Weather
Wind
Wind direction
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Summary:Aside from the influence of forcing from above on the ionosphere during space weather, forcing from below also have significant influence on the ionosphere. This study investigates responses of the equatorial ionization anomaly (EIA) in the African and American longitudinal sectors to the combined effects of 2014 Sudden Stratospheric Warming (SSW) events and geomagnetic storms that coexisted with them. The study locations cover ±40° geomagnetic latitudes in both sectors. A multiinstrument approach with models was adopted. During the SSW events, a hemispherical asymmetry in TEC distribution was observed, with higher plasma ionization in the Northern Hemisphere (NH). Generally, in both sectors, EIA crests locations shifted to higher latitudes during peak phases of SSW, except in the SH of the African sector, where crests locations shifted to lower latitudes. Reversal of stratospheric zonal mean wind direction supported reversed fountain effect. TEC responded positively to SSW peak phases and daytime or nighttime orientation of Prompt Penetration Electric Field (PPEF) and PPEF strength played major role on TEC responses to storms. PPEF values were generally weak, but comparatively higher in the American sector. TEC were predominant in the American sector than the African sector due to the comparative higher electrodynamics over the American sector. EIA crests were generally located at higher latitudes on the days of SSW peaks than on the days of geomagnetic storms, except in the NH of the American sector. In both sectors, geomagnetic storms modified ionospheric irregularities by weakening or enhancing them, while the major SSW event weakened irregularities. Plain Language Summary We investigated the responses of the EIA in the African and American sectors to the combined effects of 2014 SSW events and the geomagnetic storms that coexisted with them. We chose the study locations to cover ±40° geomagnetic latitudes in both sectors. We adopted a multiinstrument approach with models. Our results showed that the EIA crests locations in the African sector shifted from lower latitudes on pre‐SSW days to higher latitudes on minor SSW peak days in the NH. In the SH, these crests locations shifted from higher latitudes on pre‐SSW days to lower latitudes on SSW peak days, except on the day of the major SSW peak when the crest location shifted from lower latitude on pre‐SSW days to higher latitude on SSW peak days. In the American sector, EIA crest locations shifted from
ISSN:1542-7390
1539-4964
1542-7390
DOI:10.1029/2021SW002812