Physics
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..103..231m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 103, no. 2, 1986, p. 231-234.
Physics
1
Electron Transitions, Resonance Lines, Solar Spectra, Wavelengths, Beryllium, Calcium, Solar Flares
Scientific paper
The experimentally known energies of the 1s22s→1s2s(1S,3S)3p transitions are considered for lithium to calcium. Their differences from the corresponding He-like resonances are fitted to the atomic number by means of a polynomical function and, through interpolation, the wavelengths for nitrogen to sodium are calculated.
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