Fe XIV and other line identifications in the solar EUV spectrum

Details Fe XIV and other line identifications in the solar EUV spectrum Fe XIV and other line identifications in the solar EUV spectrum

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..135..343k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 135, Oct. 1991, p. 343-351.

Physics

3

Extreme Ultraviolet Radiation, Line Spectra, Solar Flares, Solar Spectra, Ultraviolet Spectra, Aluminum, Energy Levels, Iron, Spectrum Analysis

Scientific paper

A number of solar extreme ultraviolet lines, previously unidentified or given assignments at the time of observations, 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 wavelenghts in the Ne I sequence is included.

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