On the behaviour of some visible and infrared atomic hydrogen lines in facular models

dc.contributor.author	Bondal, K. R.
dc.contributor.author	Gaur, V. P.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-02-24T07:09:26Z
dc.date.available	2010-02-24T07:09:26Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/580
dc.description.abstract	The behaviour of line profiles in the wings of the Balmer, Paschen, and Brackett lines (alpha to delta) has been theoretically investigated in five facular models at disc centre. These profiles have been compared amongst the chosen facular models, and also compared with the photospheric observations. We find that these profiles can distinguish amongst different facular models. It is improving the existing facular models. Efforts should also be made to study faculae right from the ultraviolet to far-infrared.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	basi14-211
dc.subject	Facular Models, Line Profiles, Sun	en_US
dc.title	On the behaviour of some visible and infrared atomic hydrogen lines in facular models	en_US
dc.type	Article	en_US