Abstract
Abstract. This study presents statistical quantification of the correlation between
the equatorial electrojet (EEJ) and the occurrence of the equatorial ionisation
anomaly (EIA) over the East African sector. The data used were for quiet
geomagnetic conditions (Kp ≤ 3) during the period 2011–2013. The
horizontal components, H, of geomagnetic fields measured by magnetometers
located at Addis Ababa, Ethiopia (dip lat. ∼1∘ N), and Adigrat,
Ethiopia (dip lat. ∼6∘ N), were used to determine the EEJ
using differential techniques. The total electron content (TEC) derived from Global
Navigation Satellite System (GNSS) signals using 19 receivers located along
the 30–40∘ longitude sector was used to determine the EIA
strengths over the region. This was done by determining the ratio of TEC over
the crest to that over the trough, denoted as the CT : TEC ratio. This technique
necessitated characterisation of the morphology of the EIA over the region. We
found that the trough lies slightly south of the magnetic equator
(0–4∘ S). This slight southward shift of the EIA trough
might be due to the fact that over the East African region, the general
centre of the EEJ is also shifted slightly south of the magnetic equator. For the
first time over the East African sector, we determined a threshold daytime
EEJ strength of ∼ 40 nT that is mostly associated with prominent EIA
occurrence during a high solar activity period. The study also revealed that
there is a positive correlation between daytime EEJ and EIA strengths, with a
strong positive correlation occurring during the period 13:00–15:00 LT. Keywords. Ionosphere (equatorial ionosphere)
Subject
Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Geology,Astronomy and Astrophysics
Cited by
10 articles.
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