Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/37820
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dc.contributor.authorChatterjee, S. K.-
dc.contributor.authorBandyopadhyay, A. K.-
dc.contributor.authorGuhathakurta, B. K.-
dc.contributor.authorBandyopadhyay, P.-
dc.date.accessioned2016-11-29T06:41:57Z-
dc.date.available2016-11-29T06:41:57Z-
dc.date.issued1974-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37820-
dc.description248-252en_US
dc.description.abstractScintillations of signals from a number of geostationary satellites (ATS-1, ATS-3 and the Canary Bird) were observed from Huancayo-a magnetic equatorial station in the American zone. The observations made during January 1967 to December 1968 are compared with those obtained at an African equatorial station, namely, Legon. The comparison shows some differences. Particularly remarkable are the seasonal patterns at the two places. The pattern at Huancayo shows a predominantly annual periodicity while that at Legon shows a primarily semi-annual variation. These differences are described here and discussed as zonal effects.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.03(3) [September 1974]en_US
dc.titleRegional Differences in Ionospheric Scintillation near the Magnetic Equatoren_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.03(3) [September 1974]

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