On the Solar Limb Darkening in the Wings of Some Atomic Hydrogen Lines

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/925

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DC Field	Value	Language
dc.contributor.author	Bondal, K. R	-
dc.contributor.author	Gaur, V. P	-
dc.contributor.author	Pande, M. C	-
dc.date.accessioned	2006-04-10T10:32:32Z	-
dc.date.available	2006-04-10T10:32:32Z	-
dc.date.issued	1987-03	-
dc.identifier.citation	BASI, Vol. 15, No. 1, pp. 13-17	en
dc.identifier.uri	http://hdl.handle.net/2248/925	-
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 delta lamda = 5, 10, 20 and 30 A has been theoretically investigated in three photospheric modles. 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
dc.format.extent	384827 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of Indian	en
dc.subject	Photospheric modles	en
dc.subject	Hydrogen lines	en
dc.subject	Limb darkening	en
dc.title	On the Solar Limb Darkening in the Wings of Some Atomic Hydrogen Lines	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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