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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5139
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dc.contributor.authorRamanathan, A. S-
dc.date.accessioned2010-06-08T16:23:20Z-
dc.date.available2010-06-08T16:23:20Z-
dc.date.issued1954-
dc.identifier.citationZeitschrift für Astrophysik, Vol. 34, pp. 169 - 172en
dc.identifier.urihttp://hdl.handle.net/2248/5139-
dc.description.abstractThe ratio of umbral intensity to photospheric intensity as a function of wavelength has been studied in the case of four fairly large spots in the wavelength range 4000A - 6500A. The relative spectrophotometric gradient has been evaluated for each spot.en
dc.language.isoenen
dc.publisherSpringer-Verlagen
dc.rights© Springer-Verlagen
dc.subjectSunspot Umbraeen
dc.titleRadiation Flux in Sunspot Umbraeen
dc.typeArticleen
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