Molecular abundances in sunspots

dc.contributor.author	Gaur, V. P.
dc.contributor.author	Pande, M. C.
dc.contributor.author	Tripathi, B. M.
dc.date.accessioned	2011-12-09T05:01:40Z
dc.date.available	2011-12-09T05:01:40Z
dc.date.issued	1973
dc.identifier.uri	http://hdl.handle.net/123456789/880
dc.description.abstract	The results of the dissociation equilibrium calculations for Zwaan’s sunspot model are given. It appears that many di-and tri-atomic molecules form in sufficient abundances in the spots. It is suggested that for assessing the differences between the physical conditions of various sunspot models the locations of various molecules on the average geometrical depth of formation versus temperature (at that depth) curve can serve as a theoretical criterion.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	bac24-138
dc.subject	Sunspots, Zwaan’s sunspot model	en_US
dc.title	Molecular abundances in sunspots	en_US
dc.type	Article	en_US