Show simple item record Sinha, K. Joshi, G. C. Pande, M. C. 2011-09-21T06:19:54Z 2011-09-21T06:19:54Z 1976
dc.identifier.citation This article has been taken from ADS en_US
dc.description.abstract The theoretical estimates of the abundances and intensities of the fraunhofer lines for various atomic and molecular species facilitate identification and clarify the role of blending produced by the nearby lines in the solar spectrum. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries basi4-75
dc.subject Molecules species en_US
dc.title SH on the sun en_US
dc.type Article en_US

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