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	2006-04-10T09:27:33Z
dc.date.available	2006-04-10T09:27:33Z
dc.date.issued	1986-12
dc.identifier.citation	BASI, Vol. 14, No. 4, pp. 210-216	en
dc.identifier.uri	http://hdl.handle.net/2248/919
dc.description.abstract	The behavior 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 disk center. These profiles have been compared amongst the chosen facular models, and also compared with the photospheric observations. It is found that these profiles can distinguish amongst different facular models. It is suggested that low-noise high resolution spectra of these lines can help in improving the existing facular models	en
dc.format.extent	590113 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	Facular models	en
dc.subject	Line profiles	en
dc.subject	Sun	en
dc.title	On the behaviour of some visible and infrared atomic hydrogen lines in facular models	en
dc.type	Article	en