1 2 1.828e-01 0.000e+00 -1 9 2 1.271e+00 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 1.575e+00 1.494e+00 1.411e+00 1.400e+00 1.393e+00 1.346e+00 1.186e+00 8.340e-01 2.741e-01 1 3 1.828e-01 0.000e+00 -1 9 2 1.195e+00 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 2.345e+00 2.242e+00 2.131e+00 2.100e+00 2.097e+00 2.034e+00 1.813e+00 1.296e+00 3.549e-01 1 4 2.943e-01 0.000e+00 -1 9 2 5.550e-01 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 3.916e-01 4.454e-01 5.172e-01 5.629e-01 5.918e-01 6.000e-01 5.589e-01 4.099e-01 9.484e-02 1 5 2.943e-01 0.000e+00 -1 9 2 6.488e-01 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 8.102e-01 9.268e-01 1.062e+00 1.146e+00 1.194e+00 1.187e+00 1.080e+00 7.554e-01 1.761e-01 2 3 1.000e-03 0.000e+00 -1 9 2 1.909e+02 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 4.300e+00 4.435e+00 4.600e+00 4.662e+00 4.733e+00 4.857e+00 4.822e+00 3.895e+00 1.279e+00 2 4 1.115e-01 0.000e+00 -1 9 2 1.589e+00 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 1.690e+00 1.674e+00 1.692e+00 1.652e+00 1.629e+00 1.651e+00 1.666e+00 1.520e+00 1.145e+00 2 5 1.115e-01 0.000e+00 -1 9 2 1.589e+00 0.000e+00 1.250e-01 2.500e-01 3.750e-01 5.000e-01 6.250e-01 7.500e-01 8.750e-01 1.000e+00 2.481e+00 2.442e+00 2.434e+00 2.380e+00 2.373e+00 2.398e+00 2.364e+00 2.036e+00 1.257e+00 3 4 1.115e-01 0.000e+00 -1 5 2 1.960e+00 0.000e+00 2.500e-01 5.000e-01 7.500e-01 1.000e+00 1.752e+00 1.736e+00 1.702e+00 1.658e+00 9.345e-01 3 5 1.115e-01 0.000e+00 -1 5 2 1.960e+00 0.000e+00 2.500e-01 5.000e-01 7.500e-01 1.000e+00 4.443e+00 4.409e+00 4.288e+00 4.287e+00 2.888e+00 4 5 1.000e-03 0.000e+00 -1 5 2 3.702e+02 0.000e+00 2.500e-01 5.000e-01 7.500e-01 1.000e+00 1.919e+00 1.719e+00 2.016e+00 1.843e+00 6.186e-01 -1 %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 -1