On MgH line intensities in sunspot unbrae

dc.contributor.author	Sinha, K
dc.date.accessioned	2005-02-09T04:22:27Z
dc.date.available	2005-02-09T04:22:27Z
dc.date.issued	1982-09
dc.identifier.citation	BASI, Vol. 10, No. 3, pp. 223-233	en
dc.identifier.uri	http://hdl.handle.net/2248/344
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 (Triangle Nu not = 0) calculated by Kirby et al. (1979) is steressed.	en
dc.format.extent	747480 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	sunspot umbrae	en
dc.subject	MgH	en
dc.title	On MgH line intensities in sunspot unbrae	en
dc.type	Article	en