On the behaviour of some visible and infrared atomic hydrogen lines in facular models

Details On the behaviour of some visible and infrared atomic hydrogen lines in facular models On the behaviour of some visible and infrared atomic hydrogen lines in facular models

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986basi...14..211b&link_type=abstract

Astronomical Society of India, Bulletin, vol. 14, Dec. 1986, p. 211-216.

Astronomy and Astrophysics

Astronomy

1

Faculae, Hydrogen Atoms, Infrared Spectra, Solar Spectra, Stellar Models, Visible Spectrum, Balmer Series, High Resolution, Low Noise, Paschen Series

Scientific paper

The behaviour 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 disc centre. These profiles have been compared amongst the chosen facular models, and also compared with the photospheric observations. The authors find 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.

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