Singh, Lakha and Tyagi, Tuhi Ram and Somayajulu, YV and Vijayakumar, PN and Dabas, RS and Loganadham, B and Ramakrishnan, S and Rao, Rama PVS and Dasgupta, A and Navneeth, G and Klobuchar, JA and Hartmann, GK (1989) A multi-station satellite radio beacon study of ionospheric variations during total solar eclipses. In: Journal of Atmospheric and Terrestrial Physics, 51 (4). pp. 271-278.Full text not available from this repository.
Faraday rotation data obtained at Delhi, Kurukshetra, Hyderabad, Bangalore, Waltair, Nagpur and Calcutta during the total solar eclipse of 16 February 1980 and at Delhi during the total solar eclipse of 31 July 1981 have been analysed to detect the gravity waves generated by a total solar eclipse as hypothesized by Chimonas and Hines (1970, J. geophys. Res. 75, 875). 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.
|Item Type:||Journal Article|
|Additional Information:||Copyright of this article belongs to Elsevier Science.|
|Department/Centre:||Division of Mechanical Sciences > Aerospace Engineering (Formerly, Aeronautical Engineering)|
|Date Deposited:||13 Aug 2010 07:15|
|Last Modified:||13 Aug 2010 07:15|
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