Abstract
Predicted equivalent widths and profiles of facular CN lines are used here as a diagnostic tool for different model atmospheres.
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Tripathi, B.M., Sinha, K. Cyanogen lines and facula models. Sol Phys 106, 43–46 (1986). https://doi.org/10.1007/BF00161352
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DOI: https://doi.org/10.1007/BF00161352