Cyanogen lines and facula models

Details Cyanogen lines and facula models Cyanogen lines and facula models

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..106...43t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 106, July 1986, p. 43-46.

Physics

3

Cyanogen, Faculae, Solar Atmosphere, Solar Spectra, Spectral Line Width, Stellar Models, Absorption Spectra, Line Shape

Scientific paper

Comparisons are made between the equivalent widths of CN lines as calculated with different facular models and widths predicted with a photospheric model. Accurate interpretation of CN data is necessary for mapping minimum temperature regions of the solar atmosphere. Three homogeneous and three fine-structure models were, with the photospheric model of Holweger and Mueller (1974), applied to 22 lines of the (0-0) band of the red system and 16 lines of the (0-0), (1-1) and (2-2) bands of the violet system. Data plots are provided for the values obtained.

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