On the Zeeman splitting of high N recombination lines

Details On the Zeeman splitting of high N recombination lines On the Zeeman splitting of high N recombination lines

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....82..388g&link_type=abstract

Astronomy and Astrophysics, vol. 82, no. 3, Feb. 1980, p. 388.

Astronomy and Astrophysics

Astrophysics

3

Line Spectra, Radiative Recombination, Solar Spectra, Zeeman Effect, Carbon, Helium, Hydrogen

Scientific paper

The Zeeman splitting pattern of high-n alpha and beta lines of H II, He II, and Cu II ions is calculated rigorously. All allowed transitions are taken into account, together with the corresponding strengths for Russel-Saunders coupling, and the allowed fine structure transitions, the corresponding Lande factors, and the strengths are obtained by the application of selection rules. It is found that for principle quantum numbers between 30 and 300, identical hydrogen-like Zeeman triplets are obtained for the alpha and beta lines of the three ions, with a Lande factor generally equal to 1 and triplet components of equal strength.

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