On MgH line intensities in sunspot umbrae

dc.contributor.author	Sinha, K.
dc.date.accessioned	2010-07-05T06:47:34Z
dc.date.available	2010-07-05T06:47:34Z
dc.date.issued	1982
dc.identifier.citation	This article is downloaded from ADS site	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/682
dc.description.abstract	The line intensities of the umbral MgH molecules reported by Sotirovski (1971) are re-analysed utilizing the latest laboratory data. It appears probable that because of a neglect of the role of blurring in producing stray light, Sotirovski’s (1971) results are under estimated. The need of a laboratory check upon the theoretical oscillator strengths of the weak bands (∆υ ≠ 0) calculate by Kirby et al. (1979) is stressed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi10-223
dc.subject	Sunspot umbrae - MgH	en_US
dc.title	On MgH line intensities in sunspot umbrae	en_US
dc.type	Article	en_US