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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1592
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dc.contributor.authorPant, P-
dc.date.accessioned2007-05-17T05:13:30Z-
dc.date.available2007-05-17T05:13:30Z-
dc.date.issued1994-
dc.identifier.citationBASI, Vol. 22, No. 2, pp. 159-163en
dc.identifier.urihttp://hdl.handle.net/2248/1592-
dc.description.abstractThe solar flares during 1977 September have been analyzed in the light of their sudden phase anomalies (SPA) signals over long propagation paths. The analyzed data show an apparent linear relation between log (sec chi) and Delta h. Directional effect on the propagation path for VLF signals has been utilized for estimating the effective recombination coefficient and other related parameters for ionospheric D-region during these flares.en
dc.format.extent293416 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar flaresen
dc.titleSudden phase anomalies during solar flaresen
dc.typeArticleen
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