Wavelength predictions for the 1s(2)2p-1s2p3p satellite transitions

Details Wavelength predictions for the 1s(2)2p-1s2p3p satellite transitions Wavelength predictions for the 1s(2)2p-1s2p3p satellite transitions

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..108..221m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 108, no. 2, 1987, p. 221-225.

Mathematics

1

Electron Orbitals, Electron Transitions, Solar Flares, Wavelengths, Functions (Mathematics), Lithium, Polynomials, Potassium

Scientific paper

The energy differences between 1s(2)2p to 1s2p3p transitions and the corresponding 1s(2) to 1s3p resonances have been determined by means of a polynomial function of the atomic number. Good agreement between results and experimental data from lithium to potassium is found. Values for nitrogen to sodium and argon have been interpolated, and values for calcium have been extrapolated. In the case of 2S, the lines are blended with 1s(2)2s to 1s2s3p in some spectra, possibly affecting the results.

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