TY - JOUR
T1 - Classification of X-Ray Spectra from Laser Produced Plasmas of Atoms from Tm to Pt in the Range 6-9 Å
AU - Mandelbaum, P.
AU - Klapisch, M.
AU - Bar-Shalom, A.
AU - Schwob, J. L.
AU - Zigler, A.
PY - 1983/1/1
Y1 - 1983/1/1
N2 - X-ray spectra of highly ionized tungsten and neighbouring atoms (Tm, Yb, Hf, Ta, W, Re and Pt) has been observed from laser produced plasmas in the λ = 6-9 A range. Beside the prominent lines of the Ni I-like ions, lines belonging to Co I (3d 9-3d 84p), Cu I (3d 104s-3d 94s4p, 3d 104p-3d 94p 2) and Zn I-like ions (3d 104s 2-3d 94s 24p, 3d 104s4p-3d 94s4p 2) have been identified. Classification was based on isoelectronic sequence analysis and on comparison with ab-initio relativistic calculations. A collisional-radiative model of the Cu I-like ions in the plasma is used to show that the contribution of the 3d 104d-3d 94p4d and 3d 104f-3d 94f4p transition arrays to the 3d-4p spectrum is small. The importance of configuration interaction is pointed out. Computations agree with measurements within experimental uncertainty.
AB - X-ray spectra of highly ionized tungsten and neighbouring atoms (Tm, Yb, Hf, Ta, W, Re and Pt) has been observed from laser produced plasmas in the λ = 6-9 A range. Beside the prominent lines of the Ni I-like ions, lines belonging to Co I (3d 9-3d 84p), Cu I (3d 104s-3d 94s4p, 3d 104p-3d 94p 2) and Zn I-like ions (3d 104s 2-3d 94s 24p, 3d 104s4p-3d 94s4p 2) have been identified. Classification was based on isoelectronic sequence analysis and on comparison with ab-initio relativistic calculations. A collisional-radiative model of the Cu I-like ions in the plasma is used to show that the contribution of the 3d 104d-3d 94p4d and 3d 104f-3d 94f4p transition arrays to the 3d-4p spectrum is small. The importance of configuration interaction is pointed out. Computations agree with measurements within experimental uncertainty.
UR - http://www.scopus.com/inward/record.url?scp=0001655860&partnerID=8YFLogxK
U2 - 10.1088/0031-8949/27/1/005
DO - 10.1088/0031-8949/27/1/005
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AN - SCOPUS:0001655860
SN - 0031-8949
VL - 27
SP - 39
EP - 53
JO - Physica Scripta
JF - Physica Scripta
IS - 1
ER -