On the infrared opacity of sunspots

dc.contributor.author	Joshi, G. C.
dc.contributor.author	Punetha, L. M.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2011-01-11T06:02:44Z
dc.date.available	2011-01-11T06:02:44Z
dc.date.issued	1979
dc.identifier.citation	This article is taken from ADS database	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/774
dc.description.abstract	In the umbral atmosphere the depth dependence of the opacity due to the vibration rotation bands of various abundant molecules in the wavelength region 1µm to 10µm has been calculated. In the higher layers of the umbral atmosphere, the molecular opacity seems to dominate the opacity due to the negative hydrogen ion.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	sp64-255
dc.subject	Sunspots	en_US
dc.title	On the infrared opacity of sunspots	en_US
dc.type	Article	en_US