Multiplet Structure and Zeeman Effect

Abstract
Houston's method as applied to triplets and singlets cannot account for any inversions in the triplet terms. This is probably due to the fact that spin-spin and mutual spin-orbit interactions are neglected. The results of Houston's and Goudsmit's work are applied to the Zeeman effects of the spectra of Sn III and Sb I, and the agreement is found to be very satisfactory.

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