Line Profile Analysis of Carbon Molecules in the Sun

dc.contributor.author	Nirupama, Raghavan
dc.date.accessioned	2006-04-06T10:19:44Z
dc.date.available	2006-04-06T10:19:44Z
dc.date.issued	1968-09
dc.identifier.citation	KOB No 186	en
dc.identifier.uri	http://hdl.handle.net/2248/841
dc.description.abstract	Thirteen molecular lines of CN, C/sub2/ and CH have been photoelectrically observed at six disc positions each. The observed trends fall into two categories; one for strong lines and another for weak lines, irrespective of the molecule of their origin. Detailed profile calculations have been made for six selected lines. LTE methodology and an anisotropic model of turbulence have been assumed.	en
dc.format.extent	720352 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kodaikanal Observatory	en
dc.subject	Carbon Molecules	en
dc.subject	Molecular Lines	en
dc.title	Line Profile Analysis of Carbon Molecules in the Sun	en
dc.type	Article	en