Vibration - rotation bands of SiH and MgH in sunspot spectra

dc.contributor.author	Sinha, K.
dc.contributor.author	Joshi, G. C.
dc.date.accessioned	2010-07-06T06:37:40Z
dc.date.available	2010-07-06T06:37:40Z
dc.date.issued	1982
dc.identifier.citation	This article is downloaded from ADS site	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/690
dc.description.abstract	We have calculated the equivalent widths of the vibration-rotation bands of SiH and MgH molecules for a possible detection in the sunspot spectrum. Five different models were utilized and the results obtained with and without using the line haze opacity discussed by Joshi et al. (1979). It is found that the P₁ and the P₂ branches of SiH and the R branch of MgH lie in a region less dominated by the line haze opacity and consequently can be detected.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi10-329
dc.subject	SiH molecules, MgH molecules, Sunspot spectra	en_US
dc.title	Vibration - rotation bands of SiH and MgH in sunspot spectra	en_US
dc.type	Article	en_US