On the presence of SH in the sunspot spectrum

dc.contributor.author	Joshi, G. C.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2011-11-09T04:45:24Z
dc.date.available	2011-11-09T04:45:24Z
dc.date.issued	1979
dc.identifier.citation	This article is downloaded from ADS article services	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/856
dc.description.abstract	The expected equivalent widths of individual rotational lines of the most intense Q₂ branch of the 0-0 band of the A²∑-X² пi, system of S³²H and S³⁴ H have been calculated in the umbral spectrum for five disk positions using Zwaan’s (1974) sunspot model. Percentage abundance of S³⁴ in the terrestrial case has been considered valid in our calculations.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp62-69
dc.subject	SH systems, Sunspots	en_US
dc.title	On the presence of SH in the sunspot spectrum	en_US
dc.type	Article	en_US