Weak cyanogen lines in the solar spectrum in the 4139 A-4215 A region

dc.contributor.author	Porfir`eva, G. A
dc.date.accessioned	2006-04-10T05:55:55Z
dc.date.available	2006-04-10T05:55:55Z
dc.date.issued	1986-03
dc.identifier.citation	BASI, Vol. 14, No. 1, pp. 45-47	en
dc.identifier.uri	http://hdl.handle.net/2248/906
dc.description.abstract	The identification reliability of solar spectrum cyanogen lines in the 4139-4215 A region is considered in connection with the study of velocity fields by means of line profile analysis. The identification of most of the lines selected by Punetha and Joshi (1984) is found to be questionable, invalidating the Doppler width/equivalent width relation suggested for weak cyanogen lines. Seven lines cannot be considered pure cyanogen lines, and five lines contain blends of cyanogen lines with different rotation quantum numbers but with coinciding wavelengths. SiH must also be taken into account in the identification of five other solar lines	en
dc.format.extent	268497 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	Sun	en
dc.subject	Molecular Lines	en
dc.subject	CN line	en
dc.subject	Velocity fields	en
dc.title	Weak cyanogen lines in the solar spectrum in the 4139 A-4215 A region	en
dc.type	Article	en