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On the presence of SH in the sunspot spectrum

Show simple item record Joshi, G. C. Pande, M. C. 2011-11-09T04:45:24Z 2011-11-09T04:45:24Z 1979
dc.identifier.citation This article is downloaded from ADS article services en_US
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

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