1    2      143678.16      0.000e+00      7.566e-03   3s2.3p4 3P2 - 3s2.3p4 3P1
    1    3      100354.25      0.000e+00      6.053e-07   3s2.3p4 3P2 - 3s2.3p4 3P0
    2    3      332811.93      0.000e+00      1.462e-03   3s2.3p4 3P1 - 3s2.3p4 3P0
    1    4       8581.054      0.000e+00      1.038e-01   3s2.3p4 3P2 - 3s2.3p4 1D2
    2    4       9126.103      0.000e+00      2.872e-02   3s2.3p4 3P1 - 3s2.3p4 1D2
    3    4       9383.407      0.000e+00      1.134e-05   3s2.3p4 3P0 - 3s2.3p4 1D2
    1    5       3587.055      0.000e+00      1.976e-02   3s2.3p4 3P2 - 3s2.3p4 1S0
    2    5       3678.902      0.000e+00      1.297e+00   3s2.3p4 3P1 - 3s2.3p4 1S0
    4    5       6163.541      0.000e+00      2.416e+00   3s2.3p4 1D2 - 3s2.3p4 1S0
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%filename: cl_2.wgfa
%observed energy levels: Fuhr, J.R., et al., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data
%A-values: From SSTRUCT calculation. See comments below.
%comments: The A-values were derived using the code SSTRUCT, with a model of the 
   Cl II ion that contained the following 14 configurations:

   3s2.3p4
   3s.3p5
   3s2.3p3.3d
   3s2.3p3.4l  (l=s,p,d,f)
   3s2.3p3.5l  (l=s,p,d,f,g)
   3s2.3p3.6l  (l=s,p)

   Note that SSTRUCT is not best suited to ions with low charges, and 
   the derived A-values may not be good. However, there are no other values 
   in the literature.

% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%  P.R. Young - 11-Jun-2002
%File processed with wgfa_tidy by pryoung on  6-Mar-2019
 -1