| dc.description.abstract |
Variability of the Earth’s ionosphere is a threat for applications that depend on trans-ionospheric
propagating radio waves. Characterisation of its variability is the first step to make correction.
In this thesis, a sudden ionospheric disturbance (SuperSID) monitor has been deployed at Bahir
Dar, Ethiopia and the variability of the ionosphere due to solar events is investigated using the
SuperSID monitor and the recently launched Swarm satellite data. The VLF signal strength data
collected by SuperSID and in situ ion density observed by Swarm have been analysed. Plots
of VLF signal strength data showed the daytime and night-time variations of the radio signal
strength that are results of the variability of the ionosphere in these time intervals. The signal
strength variations are captured as sunset and sunrise signatures with sharp rise and sharp drop
of the signal strength respectively.
Our analysis of the Swarm satellite data also depicted that from 7.35-9.61 UT of 22 June, 2015,
the dayside ionosphere showed suppressed EIA while the nightside is strengthened indicating the
first CME of the day had resulted a disturbance dynamo. However, from 13.55-22.14 UT the
PPEF was the dominant driver of the variability. Hemispheric asymmetry of geomagnetic effect
was also observed during this event. Moreover, the EIA in the Pacific sector was the strongest
of all during the June 22, 2015 geomagnetic storm while the African sector had the highly sup-
pressed EIA in the daytime. Comparison of the daytime and nighttime recovery showed the
nighttime ionosphere has recovered sooner than the daytime. |
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