dc.description.abstract |
Scintillations are the effect of irregular electron density on the propagation of electromagnetic
signals through the ionosphere. The scintillating signals change phase unexpectedly and vary
rapidlyinamplitude. Thisstudyexaminesthetemporalcharacteristicsofthephaseandamplitude
scintillation occurrence during intense geomagnetic storm periods in the year 2015. Scintillation
indices(S4 andσφ)dataobtainedfromtwohigh-rateGlobalNavigationSatelliteSystem(GNSS)
receiver stations located at Bahir Dar University, Ethiopia was used for this purpose. In the
analysis, only GNSS signal measurements at L1, L2C, and L5C frequencies corresponding to
an elevation mask of 200 was investigated. Besides the amplitude and phase scintillation, total
electron content (TEC), and the rate of TEC index (ROTI) variations also used to investigate the
ionospheric irregularity. Results revealed that during the main phase of the storms on 17 March
2015, and on 23 June 2015, scintillation occurrence was suppressed at pre- and post-midnight
hours. On the other hand, the level of scintillation was triggered during the main phase storm
period of October 7 and December 20, 2015, at the pre-midnight hours. Comparative results
between scintillation occurrence during the storm and quiet time showed that scintillation was
more pronounced during quiet periods. It is also observed from the experimental results that the
strong scintillations occur during March equinox and December solstice, and lowest during June
solstice.
Keywords: Ionospheric scintillation, Phase and amplitude scintillations, Geomagnetic storm |
en_US |