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

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

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987basi...15...13b&link_type=abstract

Bulletin of the Astronomical Society of India V.15:1, P. 13, 1987

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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