Abstract
A revision of Schmahl's facular model is used for comparisons with the HSRA as average photosphere. On its basis many of the available data, in the visible spectrum, can be explained quantitatively.
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Caccin, B., Falciani, R. & Donati-Falchi, A. Some remarks on line weakenings in photospheric faculae. Sol Phys 35, 41–45 (1974). https://doi.org/10.1007/BF00156955
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DOI: https://doi.org/10.1007/BF00156955