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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/287
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dc.contributor.authorTyagi, Tuhi Ram-
dc.contributor.authorSingh, Lakha-
dc.contributor.authorVijaykumar, P. N-
dc.contributor.authorSomayajulu, Y. V-
dc.contributor.authorLokanadham, B-
dc.contributor.authorYellaiah, G-
dc.date.accessioned2005-02-03T04:12:47Z-
dc.date.available2005-02-03T04:12:47Z-
dc.date.issued1980-06-
dc.identifier.urihttp://hdl.handle.net/2248/287-
dc.description.abstractPreliminary results of observations, made on the eclipse day (Feb. 16, 1980) at Hyderabad, on the amplitude and phase of 136 MHz transmissions of the geostationary satellite ETS-II are presented by the eclipse. The percentage decrease in Faraday rotation showed an excellent correlation with percentage increase in optical obscuration of the Sun with a time lag of about 12 minutes. No amplitude scintillations were observed on the night of the eclipse day, though there were strong scintillations on adjacent days.en
dc.format.extent412036 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherTata Institute of Fundamental Research, Bombayen
dc.subjectTotal Solar Eclipseen
dc.subjectIonospheric variationsen
dc.subjectSatellite Radio Beacon Studyen
dc.titleSatellite Radio Beacon Study of the Ionospheric Variations at Hyderabad during the Total Solar Eclipse of Februrary 16, 1980en
dc.typeArticleen
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