Molecular line haze opacity in sunspots

dc.contributor.author	Gaur, V. P.
dc.contributor.author	Pande, M. C.
dc.contributor.author	Sah, M.
dc.date.accessioned	2011-07-08T11:30:24Z
dc.date.available	2011-07-08T11:30:24Z
dc.date.issued	1979
dc.identifier.uri	http://hdl.handle.net/123456789/824
dc.description.abstract	It has been shaown that bound-bound opacity due to electronic transitions of molecules CN, CaH, MgH and TiO explains, in first approximation, the line haze opacity postulated by Zwaan (1974) for the region 0.5 µm to 0.9 µm of the umbral spectrum.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp62-83
dc.subject	Sunspots	en_US
dc.title	Molecular line haze opacity in sunspots	en_US
dc.type	Article	en_US