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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/728
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dc.contributor.authorSujatha, N. V-
dc.contributor.authorChakraborty, P-
dc.contributor.authorMurthy, J-
dc.contributor.authorHenry, R. C-
dc.date.accessioned2006-03-13T06:49:34Z-
dc.date.available2006-03-13T06:49:34Z-
dc.date.issued2004-09-
dc.identifier.citationBASI, Vol. 32, No. 3, pp. 151-158en
dc.identifier.urihttp://hdl.handle.net/2248 /728-
dc.description.abstractThis work is the first step in a systematic effort to understand and predict the different components of the UV (912 A - 3000 A) radiation field over the entire sky. We have developed a model to predict the ISRF in the UV within a few hundred parsecs of the Sun using the Hipparcos star catalog. We have checked the model through a comparison with the observations of the Belgian/UK UV sky survey telescope (S2/68) on the ESRO TD-1 satelliteen
dc.format.extent251028 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectInterstellar radiation field (ISRF)en
dc.subjectdiffuse backgrounden
dc.titleA model of the stellar radiation field in the UVen
dc.typeArticleen
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