1.000e+03  2.000e+03  5.000e+03  1.000e+04  2.000e+04  5.000e+04  8.000e+04  1.000e+05  2.000e+05  5.000e+05  8.000e+05  1.000e+06  2.000e+06  5.000e+06  8.000e+06  1.000e+07
    1    5    1    1  1.121e+01  2.373e-09  2.308e-09  2.229e-09  2.260e-09  2.477e-09  3.699e-09  5.383e-09  6.616e-09  1.311e-08  3.087e-08  4.474e-08  5.240e-08  8.055e-08  1.282e-07  1.574e-07  1.726e-07
    1    5    2    2  2.253e-01  1.220e-14  1.370e-14  1.460e-14  1.610e-14  1.970e-14  3.620e-14  1.610e-13  4.740e-13  7.920e-12  6.850e-11  1.400e-10  1.870e-10  3.970e-10  9.830e-10  1.660e-09  2.180e-09
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Charge transfer recombination of C V.

Data for CT with H from: Liu, C.-N., Le, A.-T., & Lin, C. D. 2003, Phys. Rev. A, 68, 062702
Data for CT with He from: Yan, L. L., Wu, Y., Qu, Y. Z., Wang, J. G., & Buenker, R. J. 2013, Phys. Rev. A, 88, 022706

The total rate coefficient for CT with He has been given here as recombining into level 5. This is the dominant channel
  at solar temperatures, but cross sections in the original article show that recombination into some other states
  dominate depending on the temperature of the environment.

File prepared by R.P. Dufresne on 25-Oct-2023

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