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

Show simple item record Bondal, K. R. Gaur, V. P. Pande, M. C. 2010-02-24T06:06:00Z 2010-02-24T06:06:00Z 1987
dc.identifier.citation This article is downloaded for ADS en_US
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

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