Abstract
The detailed study of the possible presence of four [Niii] lines in solar absorption leads to an abundanceA ni = logN ni = 6.30±0.30 (in the usual scale where logN H = 12.00), in agreement with the coronal and meteoritic values.
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References
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On leave from Institut d'Astrophysique, Université de Liège.
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Grevesse, N., Swings, J.P. The solar abundance of nickel from photospheric [Niii] lines. Sol Phys 13, 19–24 (1970). https://doi.org/10.1007/BF00963938
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DOI: https://doi.org/10.1007/BF00963938