Abstract

New measurements for the transitions 3s2S10-3s3p1P31 in the Mg i isoelectronic sequence and for 3s23p6S10-3s23p53dP11 and D31 in the Ar i sequence are given for most of the elements from Cu to Mo. These measurements are compared with uniformly scaled relativistic Hartree–Fock calculations, and the wavelength differences are fit to a continuous function from which new smoothed values are derived with an estimated uncertainty of ±0.005 Å.

© 1987 Optical Society of America

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