On the solar limb darkening in the wings of some atomic hydrogen lines

dc.contributor.author	Bondal, K. R.
dc.contributor.author	Gaur, V. P.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-02-24T06:06:00Z
dc.date.available	2010-02-24T06:06:00Z
dc.date.issued	1987
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/576
dc.description.abstract	The centre-to-limb behaviour of the first four lines of the Balmer, Paschen, and Brackett series of atomic hydrogen at selected distances from the line centre, i.e. at Δλ = 5, 10, 20, and 30 Å has been theoretically investigated in three photospheric models. The results have been compared with observations of David (1961) for the Balmer lines, the corresponding observations for Paschen and Brackett lines not being available in published sources. After a detailed comparison of the computed results with the observations, it is concluded that limb-darkening data in the wings of hydrogen series lines can distinguish amongst the various photospheric models.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi15-13
dc.subject	Photospheric models - Hydrogen lines, Limb darkening	en_US
dc.title	On the solar limb darkening in the wings of some atomic hydrogen lines	en_US
dc.type	Article	en_US