Abstract:During the total solar eclipse period on 24 October 1995, the ionospheric data derived from Faraday rotation, differential Doppler frequency shift, and HF Doppler sounding at Lunping Observatory were used to detect the traveling ionospheric disturbances associated with the solar eclipse of that day. These observed ionospheric disturbances were characterized by quasi periodic wave-like trains lasting for several cycles with wavelengths of around 193 km, periods of around 12-14 min and propagated with a hori zon… Show more
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