Abstract
A number of solar extreme ultraviolet lines, previously unidentified or given assignments at the time of observation, are found to be coincident in wavelength with transitions recently identified as aluminum-like or magnesium-like in the laboratory. Three tables summarize the results of this comparison, which does not imply positive identifications but suggests that several assignments may be valid. Additional assignments are proposed in other ions and a revised table of predicted and observed forbidden line wavelengths in the Ne i sequence is included.
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Kastner, S.O. Fe xiv and other line identifications in the solar EUV spectrum. Sol Phys 135, 343–351 (1991). https://doi.org/10.1007/BF00147506
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DOI: https://doi.org/10.1007/BF00147506