Evolution of sunspots seen in molecular lines. Ⅱ

dc.contributor.author	Sinha, K.
dc.contributor.author	Tripathi, B. M.
dc.date.accessioned	2010-01-15T05:41:57Z
dc.date.available	2010-01-15T05:41:57Z
dc.date.issued	1991
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/438
dc.description.abstract	Utilizing the model atmospheres proposed by Sobotka for umbrae of different sizes and those proposed by Maltby et al. for well-developed umbrae, at diffrent phased of solar activity, we examine themolecules C₂, MgH and TiO for a study of sunspot evolution.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi19-23
dc.subject	Sunspot, Spectrum, Molecules	en_US
dc.title	Evolution of sunspots seen in molecular lines. Ⅱ	en_US
dc.type	Article	en_US