belike_lfm14#c2.dat

• Spontaneous Emission: C⁺²(i) → C⁺²(j) + hv
• Electron Impact Excitation: C⁺²(i) + e → C⁺²(j) + e

 + 2         6         3        386241.(  )
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        Result of ICFT R-matrix calculation
        +++++++++++++++++++++++++++++++++++

 Calculation automated by offline ADAS code ADAS8#3

     Summary Information
     +++++++++++++++++++

 *  Ionisation energy taken from ADAS adf00 files

 *  Energy levels calculated by AUTOSTRUCTURE

 *  Radiative rates calculated by AUTOSTRUCTURE

 *  Effective collision strengths calculated by ICFT
    R-matrix calculation using target structure from
    AUTOSTRUCTURE.

     Calculation details
     +++++++++++++++++++

 The following scaling parameters on bound orbitals were used:

         1s = 1.41290
         2s = 1.49099
         2p = 1.43422
         3s = 1.20193
         3p = 1.13345
         3d = 1.27955
         4s = 1.20122
         4p = 1.12308
         4d = 1.28131
         4f = 1.43825
         5s = 1.20319
         5p = 1.11983
         5d = 1.28608
         5f = 1.44185
         5g = 1.57035
         6s = 1.20542
         6p = 1.11806
         6d = 1.29188
         7s = 1.20938
         7p = 1.11667
         7d = 1.29554

 An exchange calculation was performed up to J=11.5
 A non-exchange calculation was then performed up to J=45
 Followed by a top-up calculation to J -> infinity.

 80 continuum basis orbitals were used, giving a smallest maximum
 basis-orbital energy of 0 Rydbergs (0.000000 eV)

 A fine energy mesh of 0.000010 Z**2 Rydbergs (0.00054424 eV) was used
 between the first and last thresholds for the excitation calculation.

 A coarse energy mesh of 0.001000 Z**2 Rydbergs (0.054424 eV) was used
 from the last threshold up to 2.639706 Z**2 Rydbergs (143.6633361 eV) in the
 excitation calculation.

 A coarse energy mesh of 0.001000 Z**2 Rydbergs (0.054424 eV) was used
 from first threshold up to 2.639706 Z**2 Rydbergs (143.6633361 eV) in the
 non-exchange calculation.

 Dipole and Born limits were used from the last calculated energy points
 up to infinite energy to complete the effective collision strengths

 Produced by: Luis Fernandez-Menchero
 Date:        10/01/14
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 L. Fernandez-Menchero, G. Del Zanna, and N. R. Badnell
 Astronomy and Astrophysics 566, A104 (2014)
 DOI: 10.1051/0004-6361/201423864
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Contributors

• Luis Fernandez Menchero
• Nigel Badnell