S320p.43 — Studing Solar Flare Effects on Ionosphere Using AWESOME Receiver

Date & Time

Aug 10th at 6:00 PM until 7:30 PM




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Author(s): Famil Mustafa1, Elchin Babayev1, Ilgar Alekperov1

Institution(s): 1. Shamakhy Astrophysical Observatory named after N.Tusi

Ground based observations of Extremely Low Frequency (ELF) / Very Low Frequency (VLF) (300 Hz 30 kHz) waves are considered as an important remote sensing tool for the investigation of the ionosphere and the magnetosphere. VLF waves find their origin in various natural and artificial phenomena; the natural sources include thunderstorms, lightning and associated phenomena. Sub-ionospheric VLF transmissions propagating inside the Earth-ionosphere wave-guide is also being widely used for investigating sudden ionospheric perturbations (SIDs) in lower part of the ionosphere.