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** Atomic data from version 7 of the CHIANTI database **
%Observed energy levels (n=2): Edlen, B., 1983, Physica Scripta, 28, 51
%Observed energy levels (4-10,24,39,41,44-49,52-53,55-60,64-65,67,69-70,82,95,105,114,117,125,131,147-151):
       Fawcett, B.C., Hayes, R.W. 1987, Physica Scripta, 36, 80
%Observed energy levels (11-18,21-22,25-29,35,38,43,50-51,54,123-124,129,134,136-137,155,157,162,188-189):
       Bengtsson, P., Jupen, C., Engstrom, L., Redfors, A., Westerlind, M, 1993, Phys. Scr., 48,413
%Theoretical energy levels: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%   E. Landi - Feb 2007
%filename: s_8.wgfa
%Observed energy levels (n=2): Edlen, B., 1983, Physica Scripta, 28, 51
%Observed energy levels (4-10,24,39,41,44-49,52-53,55-60,64-65,67,69-70,82,95,105,114,117,125,131,147-151):
       Fawcett, B.C., Hayes, R.W. 1987, Physica Scripta, 36, 80
%Observed energy levels (11-18,21-22,25-29,35,38,43,50-51,54,123-124,129,134,136-137,155,157,162,188-189):
       Bengtsson, P., Jupen, C., Engstrom, L., Redfors, A., Westerlind, M, 1993, Phys. Scr., 48,413
%Theoretical energy levels: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
%Radiative data: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%   E. Landi - Feb 2007

%filename: s_8.splups
%Oscillator strengths: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
%Effective collision strengths: Witthoeft, M.C., Whiteford, A.D., & Badnell, N.R. 2007, J.Phys.B, 40, 2969
%comment: effective collision strengths are published for temperatures in the range  4.1 < Log T <  8.1
%comment: effective collision strengths are USED for temperatures in the range  4.5 < Log T <  7.3
%comment: data at very high or very low temperatures were sometimes discarded to improve the fit. At these
     temperatures the S VIII abundance is negligible under equilibrium.
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
% E. Landi - Feb 2007
 2 23
  1  2s2.2p5 2P3/2
  2  2s2.2p5 2P1/2
     100.0
     158.5
     251.2
     398.1
     631.0
    1000.0
    1584.9
    2511.9
    3981.1
    6309.6
   10000.0
   15848.9
   25118.9
   39810.7
   63095.8
  100000.0
  158489.2
  251188.7
  398107.1
  630957.6
 1000000.0
 1584892.5
 2511887.0
0
  1  2   1.61e-01
  0  0   1.61e-01
  0  0   1.61e-01
  0  0   1.61e-01
  0  0   1.62e-01
  0  0   1.62e-01
  0  0   1.63e-01
  0  0   1.64e-01
  0  0   1.66e-01
  0  0   1.69e-01
  0  0   1.74e-01
  0  0   1.81e-01
  0  0   1.93e-01
  0  0   2.10e-01
  0  0   2.35e-01
  0  0   2.65e-01
  0  0   2.91e-01
  0  0   3.05e-01
  0  0   3.09e-01
  0  0   3.08e-01
  0  0   3.00e-01
  0  0   2.76e-01
  0  0   2.39e-01
 0 0 0
  1  2   2.200e+01
  1  4        0.0
  2  2    10084.0