Molecules  in the Solar Photosphere

dc.contributor.author	Pande, M. C.
dc.contributor.author	Gaur, V. P.
dc.contributor.author	Tripathi, B. M.
dc.date.accessioned	2015-08-19T08:51:20Z
dc.date.available	2015-08-19T08:51:20Z
dc.date.issued	2015-08-19
dc.identifier.uri	http://hdl.handle.net/123456789/1216
dc.description.abstract	A consideration of the dissociation equilibrium of diatomic molecules in the Utrecht Reference Photosphere leads us to conclude that SH, SiO, CS, HF and HCl may show up in enough concentrations in the solar atmosphere. The number above photosphere for these molecules is comparable with or more than that of MgH.
dc.description.abstract	A consideration of the dissociation equilibrium of diatomic molecules in the Utrecht Reference Photosphere leads us to conclude that SH, SiO, CS, HF and HCl may show up in enough concentrations in the solar atmosphere. The number above photosphere for these molecules is comparable with or more than that of MgH.
dc.language.iso	en	en_US
dc.relation.ispartofseries	SP7-17
dc.subject	Solar atmosphere	en_US
dc.title	Molecules in the Solar Photosphere	en_US
dc.type	Article	en_US