10
 17  3    1    2  2  0.000e+00  1.828e-01
 17  3    1    3  2  0.000e+00  1.828e-01
 17  3    1    4  2  0.000e+00  2.943e-01
 17  3    1    5  2  0.000e+00  2.943e-01
 17  3    2    3  2  0.000e+00  1.000e-03
 17  3    2    4  2  0.000e+00  1.115e-01
 17  3    2    5  2  0.000e+00  1.115e-01
 17  3    3    4  2  0.000e+00  1.115e-01
 17  3    3    5  2  0.000e+00  1.115e-01
 17  3    4    5  2  0.000e+00  1.000e-03
-1
data were taken from
%filename:  cl_3.splups
%Theoretical energies: Ramsbottom, C.A., Bell, K.L., & Keenan, F.P. 2001, ADNDT, 77, 57
%Effective collision strengths: Ramsbottom, C.A., Bell, K.L., & Keenan, F.P. 2001, ADNDT, 77, 57
%Comment:  Ramsbottom et al. (2001) gave LS energies. For transitions within multiplets, an 
           energy splitting of 0.001 Ryd has been assumed.
           The spline fits are accurate to 0.56% or better over the temperature range 7500 to 250,000 K.
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
% %   Peter Young, 1-Dec-2010
%  E.Dz. for KAPPA  08-AUG-2019
-1