Abstract
The red shift and central intensity are given for eleven spectral lines having an observed reduced equivalent widthV ranging fromV=15 toV=200. The computations have been repeated for eight values of the scattering thickness of the chromosphere, from\(\tau ' = 0.2/\sqrt 3 \) to\(\tau ' = 1.4/\sqrt 3 \). A theoretical interpretation of measurements in the Sun is also given.
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References
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Missana, M., Piana, A. The compton effect in the chromosphere, II. Astrophys Space Sci 43, 129–134 (1976). https://doi.org/10.1007/BF00640561
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DOI: https://doi.org/10.1007/BF00640561