A multi-station satellite radio beacon study of ionospheric variations during total solar eclipses

Computer Science – Sound

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Gravity Waves, Ionospheric Disturbances, Satellite Sounding, Solar Eclipses, Solar Terrestrial Interactions, Faraday Effect, Radio Beacons

Scientific paper

Faraday rotation data obtained at Delhi, Kurukshetra, Hyderabad, Bangalore, Waltair, Nagpur and Calcutta during the total solar eclipse of February 16, 1980 and at Delhi during the total solar eclipse of July 31, 1981 have been analyzed to detect the gravity waves generated by a total solar eclipse as hypothesized by CHIMONAS and HINES (1970). It has been found that gravity waves can be generated by a total solar eclipse but their detection at ionospheric heights is critically dependent on the location of the observing station in relation to the eclipse path geometry. The distance of the observing station from the eclipse path should be more than 500 km in order to detect such gravity waves.

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