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The scintillation activity observed on solstice days was relatively low and almost constant throughout the day with low post-sunset activity levels.
Abdu et al. (2015) investigated the role of eastward and upward propagating fast (FK) and ultrafast Kelvin (UFK) waves in the day-to-day variability of equatorial evening PRE and post-sunset generation of ESF.
The diurnal analysis revealed that the ionospheric critical frequency (foF2) is more susceptible to variability during the night-time than the day-time, with two peaks in the range; 18 38% during post-sunset hours and 35 55% during post-midnight hours.
It may be noted that the larger PRE amplitude around the day 290 was responsible for the larger intensity and earlier onset time of the post-sunset ESF.
The post-sunset enhancements in the vertical drift of the equatorial F-layer are also reduced significantly from their quiet day patterns and the subsequent occurrence of Spread-F and scintillations is inhibited.
The post-sunset enhancement and its reversal are also discussed.
The vivid ash-tinged sunsets, and the post-sunset horizon rainbows of purple and passion fruit and salmon-red, were said to be the most memorable.
post-sunset rise.
Results are presented for post-sunset (left panel) and post-midnight (right panel) time.
In general, the equatorial plasma bubbles have been regarded as the typical post-sunset phenomena.
Around June 2014 and July 2015, the equator crossings are also during the post-sunset hours.
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