Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/37805
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSastry, Ch. V.-
dc.contributor.authorSubrahmanyan, K. R.-
dc.date.accessioned2016-11-29T06:22:16Z-
dc.date.available2016-11-29T06:22:16Z-
dc.date.issued1974-09-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37805-
dc.description196-198en_US
dc.description.abstractObservations on the occultation of the radio source Tauras A (3C 144) during June 1971 at a wavelength of 12 m are presented. It is tentatively observed that there is no strong dependence between the amount of scattering and solar activity.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.titleObservations on the Occultation of the Radio Source Tauras A by the Solar Corona during June 1971en_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.03(3) [September 1974]

Files in This Item:
File Description SizeFormat 
IJRSP 3(3) 196-198.pdf213.31 kBAdobe PDFView/Open


Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.