      1     3p6.4s                            2  S    0.5          0.000          0.000
      2     3p6.3d                            2  D    1.5      13650.190      13650.190
      3     3p6.3d                            2  D    2.5      13710.880      13710.880
      4     3p6.4p                            2  P    0.5      25191.510      25191.510
      5     3p6.4p                            2  P    1.5      25414.400      25414.400
      6     3p6.5s                            2  S    0.5      52166.930      52166.930
      7     3p6.4d                            2  D    1.5      56839.250      56839.250
      8     3p6.4d                            2  D    2.5      56858.460      56858.460
      9     3p6.5p                            2  P    0.5      60533.020      60533.020
     10     3p6.5p                            2  P    1.5      60611.280      60611.280
     11     3p6.4f                            2  F    2.5      68056.910      68056.910
     12     3p6.4f                            2  F    3.5      68057.910      68057.910
     13     3p6.6s                            2  S    0.5      70677.620      70677.620
     14     3p6.5d                            2  D    1.5      72722.230      72722.230
     15     3p6.5d                            2  D    2.5      72730.930      72730.930
     16     3p6.6p                            2  P    0.5      74484.920      74484.920
     17     3p6.6p                            2  P    1.5      74521.750      74521.750
     18     3p6.5f                            2  F    2.5      78034.390      78034.390
     19     3p6.5f                            2  F    3.5      78035.390      78035.390
     20     3p6.5g                            2  G    3.5      78164.720      78164.720
     21     3p6.5g                            2  G    4.5      78165.720      78165.720
     22     3p6.7s                            2  S    0.5      79448.280      79448.280
     23     3p6.6d                            2  D    1.5      80521.530      80521.530
     24     3p6.6d                            2  D    2.5      80526.160      80526.160
     25     3p6.6f                            2  F    2.5      83458.080      83458.080
     26     3p6.6f                            2  F    3.5      83459.080      83459.080
     27     3p6.6g                            2  G    3.5      83540.000      83540.000
     28     3p6.6g                            2  G    4.5      83541.000      83541.000
     29     3p6.8s                            2  S    0.5      84300.890      84300.890
     30     3p6.7d                            2  D    1.5      84933.650      84933.650
     31     3p6.7d                            2  D    2.5      84936.410      84936.410
     32     3p6.7f                            2  F    2.5      86727.060      86727.060
     33     3p6.7f                            2  F    3.5      86728.060      86728.060
     34     3p6.7g                            2  G    3.5      86781.140      86781.140
     35     3p6.7g                            2  G    4.5      86782.140      86782.140
     36     3p6.8d                            2  D    1.5      87671.930      87671.930
     37     3p6.8d                            2  D    2.5      87673.720      87673.720
     38     3p6.8f                            2  F    2.5      88847.310      88847.310
     39     3p6.8f                            2  F    3.5      88848.310      88848.310
     40     3p6.8g                            2  G    3.5      88884.540      88884.540
     41     3p6.8g                            2  G    4.5      88885.540      88885.540
 -1
%filename:  ca_2.elvlc
%observed energies: v.3 of the NIST Atomic Database
%theoretical energies: These were not published by Melendez et al. (2007) so the observed energies have been used.
%comment: Some of the fine structure levels arising from the same spectroscopic
   term are given the same energy value in the NIST database. For CHIANTI,
   an artificial separation of 1 cm^-1 has been applied to these levels.
% produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
%
%      Peter Young, Jan 2009
