SH on the sun

dc.contributor.author	Sinha, K.
dc.contributor.author	Joshi, G. C.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2011-09-21T06:19:54Z
dc.date.available	2011-09-21T06:19:54Z
dc.date.issued	1976
dc.identifier.citation	This article has been taken from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/844
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