Vibration-rotation bands of SiH and MgH in sunspot spectra

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/351

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DC Field	Value	Language
dc.contributor.author	Sinha, K	-
dc.contributor.author	Joshi, G. C	-
dc.date.accessioned	2005-02-09T06:25:38Z	-
dc.date.available	2005-02-09T06:25:38Z	-
dc.date.issued	1982-12	-
dc.identifier.citation	BASI, Vol. 10, No. 4, pp. 329-333	en
dc.identifier.uri	http://hdl.handle.net/2248/351	-
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 baze 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
dc.format.extent	378801 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	SiH molecules	en
dc.subject	MgH molecules	en
dc.subject	sunspot spectrum	en
dc.title	Vibration-rotation bands of SiH and MgH in sunspot spectra	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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