Solar photospheric models and the rotational temperatures of the C₂ and MgH molecules

dc.contributor.author	Singh, K.
dc.contributor.author	Shukla, D. S.
dc.contributor.author	Tripathi, B. M.
dc.date.accessioned	2011-07-08T11:14:24Z
dc.date.available	2011-07-08T11:14:24Z
dc.date.issued	1979
dc.identifier.uri	http://hdl.handle.net/123456789/822
dc.description.abstract	Four photospheric models have been utilized to derive model based rotational temperatures of the (0-0) band of the Swan system of C₂ and that of the green system of the MgH molecules. The dissociation energies were varied within reasonable limits to assess their influence on the derived temperatures. It is found that observations are not consistent with the model based results. The need for more refined photospheric models is emphasized.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi7-38
dc.subject	Solar Photospheric	en_US
dc.title	Solar photospheric models and the rotational temperatures of the C₂ and MgH molecules	en_US
dc.type	Article	en_US