Abstract

Extreme UV spectra of the gadolinium and terbium ions excited in the laser-produced plasma and vacuum spark sources were recorded in the 40–120 Å region and investigated on the basis of the Hartree–Fock calculations using Cowan code. The intense peaks in the 65–75 Å region of the vacuum spark spectra were interpreted as a manifold of the 4d104fm–4d94fm+1 transitions in the ions with a partially filled 4f shell. The drastic narrowing of these peaks was observed in the spectra of the laser-produced plasma. It was explained by a change of the 4d104fm–4d94fm+1 (m>2) transition arrays mostly contributing to the intensity of the peaks in the vacuum spark spectra for the 4–4 transitions in the simplest spectra of the 4p64dk (k=8–10) and 4d104fm (m=1–2) ground configuration ions predominantly excited in hotter laser-produced plasma. The most intense lines of the 4d104f2–4d104f5d transitions in the Gd XVII and Tb XVIII spectra were classified for the first time.

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