chv6_ic#ca12.dat

Resolved Specific Ion Data Collections

Ion
Ca12+
Temperature Range
7.281 eV → 7281 eV

ADF04

Filename
chv6_ic#ca12.dat
Full Path
adf04/copch#20/chv6_ic#ca12.dat
Download data
  • Spontaneous Emission: Ca+12(i) → Ca+12(j) + hv
  • Electron Impact Excitation: Ca+12(i) + e → Ca+12(j) + e
2s2.2p4 3p2 3P2.0 0.0 cm-1
2s2.2p4 3p1 3P1.0 25015.9 cm-1
2s2.2p4 3p0 3P0.0 29487.7 cm-1
2s2.2p4 1d2 1D2.0 91945.0 cm-1
2s2.2p4 1s0 1S0.0 180687.0 cm-1
2s.2p5 3p2 3P2.0 628533.0 cm-1
2s.2p5 3p1 3P1.0 648949.0 cm-1
2s.2p5 3p0 3P0.0 661061.0 cm-1
2s.2p5 1p1 1P1.0 869796.0 cm-1
2p6 1s0 1S0.0 1474920.0 cm-1
2s2.2p3(4s).3s 5s2 5S2.0 3332410.0 cm-1
2s2.2p3(4s).3s 3s1 3S1.0 3373580.0 cm-1
2s2.2p3(2d).3s 3d1 3D1.0 3452100.0 cm-1
2s2.2p3(2d).3s 3d2 3D2.0 3453110.0 cm-1
2s2.2p3(2d).3s 3d3 3D3.0 3459720.0 cm-1
2s2.2p3(2d).3s 1d2 1D2.0 3476610.0 cm-1
2s2.2p3(4s).3p 5p1 5P1.0 3492940.0 cm-1
2s2.2p3(4s).3p 5p2 5P2.0 3494830.0 cm-1
2s2.2p3(4s).3p 5p3 5P3.0 3499020.0 cm-1
2s2.2p3(2p).3s 3p0 3P0.0 3513600.0 cm-1
2s2.2p3(2p).3s 3p1 3P1.0 3516600.0 cm-1
2s2.2p3(2p).3s 3p2 3P2.0 3526320.0 cm-1
2s2.2p3(4s).3p 3p1 3P1.0 3532550.0 cm-1
2s2.2p3(4s).3p 3p2 3P2.0 3535550.0 cm-1
2s2.2p3(4s).3p 3p0 3P0.0 3536790.0 cm-1
2s2.2p3(2p).3s 1p1 1P1.0 3541870.0 cm-1
2s2.2p3(2d).3p 3d1 3D1.0 3592980.0 cm-1
2s2.2p3(2d).3p 3d2 3D2.0 3605070.0 cm-1
2s2.2p3(2d).3p 3d3 3D3.0 3612090.0 cm-1
2s2.2p3(2d).3p 1p1 1P1.0 3612140.0 cm-1
2s2.2p3(2d).3p 3f2 3F2.0 3616360.0 cm-1
2s2.2p3(2d).3p 3f3 3F3.0 3621840.0 cm-1
2s2.2p3(2d).3p 3f4 3F4.0 3627680.0 cm-1
2s2.2p3(2d).3p 1f3 1F3.0 3629170.0 cm-1
2s2.2p3(2d).3p 3p1 3P1.0 3659430.0 cm-1
2s2.2p3(2d).3p 3p0 3P0.0 3665240.0 cm-1
2s2.2p3(2d).3p 3p2 3P2.0 3677040.0 cm-1
2s2.2p3(2p).3p 1p1 1P1.0 3677770.0 cm-1
2s2.2p3(2p).3p 3d2 3D2.0 3682750.0 cm-1
2s2.2p3(2p).3p 3s1 3S1.0 3683480.0 cm-1
2s2.2p3(2p).3p 3d3 3D3.0 3690720.0 cm-1
2s2.2p3(2d).3p 1d2 1D2.0 3691120.0 cm-1
2s2.2p3(4s).3d 5d0 5D0.0 3698190.0 cm-1
2s2.2p3(4s).3d 5d1 5D1.0 3698360.0 cm-1
2s2.2p3(4s).3d 5d2 5D2.0 3698630.0 cm-1
2s2.2p3(4s).3d 5d3 5D3.0 3699000.0 cm-1
2s2.2p3(4s).3d 5d4 5D4.0 3699760.0 cm-1
2s2.2p3(2p).3p 3d1 3D1.0 3699900.0 cm-1
2s2.2p3(2p).3p 3p2 3P2.0 3713780.0 cm-1
2s2.2p3(2p).3p 3p1 3P1.0 3716370.0 cm-1
2s2.2p3(2p).3p 3p0 3P0.0 3716860.0 cm-1
2s2.2p3(4s).3d 3d2 3D2.0 3741730.0 cm-1
2s2.2p3(4s).3d 3d1 3D1.0 3744680.0 cm-1
2s2.2p3(4s).3d 3d3 3D3.0 3745840.0 cm-1
2s2.2p3(2p).3p 1d2 1D2.0 3750850.0 cm-1
2s2.2p3(2d).3d 3f2 3F2.0 3802460.0 cm-1
2s2.2p3(2d).3d 3f3 3F3.0 3808180.0 cm-1
2s2.2p3(2p).3p 1s0 1S0.0 3811460.0 cm-1
2s2.2p3(2d).3d 1s0 1S0.0 3811660.0 cm-1
2s2.2p3(2d).3d 3f4 3F4.0 3814740.0 cm-1
2s2.2p3(2d).3d 3g3 3G3.0 3820570.0 cm-1
2s2.2p3(2d).3d 3g4 3G4.0 3823850.0 cm-1
2s2.2p3(2d).3d 3g5 3G5.0 3828150.0 cm-1
2s2.2p3(2d).3d 3d1 3D1.0 3829220.0 cm-1
2s2.2p3(2d).3d 1g4 1G4.0 3830980.0 cm-1
2s2.2p3(2d).3d 3d2 3D2.0 3842450.0 cm-1
2s2.2p3(2d).3d 1p1 1P1.0 3845730.0 cm-1
2s2.2p3(2d).3d 3d3 3D3.0 3847900.0 cm-1
2s2.2p3(2p).3d 1d2 1D2.0 3852480.0 cm-1
2s2.2p3(2d).3d 3p2 3P2.0 3855690.0 cm-1
2s2.2p3(2d).3d 3p0 3P0.0 3858300.0 cm-1
2s2.2p3(2d).3d 3p1 3P1.0 3860120.0 cm-1
2s2.2p3(2d).3d 3s1 3S1.0 3866070.0 cm-1
2s2.2p3(2p).3d 3f3 3F3.0 3883660.0 cm-1
2s2.2p3(2p).3d 3f2 3F2.0 3887220.0 cm-1
2s2.2p3(2d).3d 1f3 1F3.0 3889920.0 cm-1
2s2.2p3(2p).3d 3f4 3F4.0 3890950.0 cm-1
2s2.2p3(2p).3d 3p0 3P0.0 3892280.0 cm-1
2s2.2p3(2p).3d 3p1 3P1.0 3896350.0 cm-1
2s2.2p3(2p).3d 3p2 3P2.0 3897020.0 cm-1
2s2.2p3(2p).3d 3d2 3D2.0 3908230.0 cm-1
2s2.2p3(2p).3d 3d1 3D1.0 3914200.0 cm-1
2s2.2p3(2p).3d 3d3 3D3.0 3915250.0 cm-1
2s2.2p3(2d).3d 1d2 1D2.0 3931720.0 cm-1
2s2.2p3(2p).3d 1f3 1F3.0 3935280.0 cm-1
2s2.2p3(2p).3d 1p1 1P1.0 3972700.0 cm-1
A+12        20        13       5845430.2
----------------------------------------------------------------------------

  Data generated from CHIANTI version 6.0

       http://www.chianti.rl.ac.uk/

  CHIANTI references
  ------------------

  Energy levels :
   %Observed energy levels (1 - 10): Edlen, 1983, Ph. Scr., 28, 51
   %Observed energy levels (4,5): Feldman, Curdt, Landi, Wilhelm, 2000, ApJ, 544, 508
   %Observed energy levels (11): from the spectrum of Acton et al 1985, ApJ, 291, 865
   %Observed energy levels (12 - 16,25 - 26): Doschek et al 1973, J.Opt.Soc.Am, 63, 1463
   %Observed energy levels (2s2.2p3.3d configuration): Fawcett & Hayes, 1975, MNRAS, 170, 185
   %theoretical energy levels: Landi, E., Bhatia, A.K., 2005, A&A, 444, 305
   %comment: theoretical energy levels come from the 24-configuration calculation in Landi & Bhatia (2005)
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi - Mar 2005

  A-values levels :
   %filename: ca_13.wgfa
   %Observed energy levels (1-10): Edlen, 1983, Ph. Scr., 28, 51
   %Observed energy levels (4,5): Feldman, Curdt, Landi, Wilhelm, 2000, ApJ, 544, 508
   %Observed energy levels (11): from the spectrum of Acton et al 1985, ApJ, 291, 865
   %Observed energy levels (12-16,25-26): Doschek et al 1973, J.Opt.Soc.Am, 63, 1463
   %Observed energy levels (2s2.2p3.3d configuration): Fawcett & Hayes, 1975, MNRAS, 170, 185
   %theoretical energy levels: Landi, E., Bhatia, A.K., 2005, A&A, 444, 305
   %A values and oscillator strengths: Landi, E., Bhatia, A.K., 2005, A&A, 444, 305
   %comment: theoretical energies and radiative data come from the 24-configuration calculation in Landi & Bhatia (2005)
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi - Apr 2005

  Collision strengths :

   %filename: ca_13.splups
   %Collision strengths: Landi & Bhatia 2005, A&A, 444, 305
   %Oscillator strengths: Landi & Bhatia 2005, A&A, 444, 305
   %comment: oscillator strengths have been taken from the 6-configuration model of Landi & Bhatia
       (2005) for consistency with the collisional calculation
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi - Mar 2005



  Added to ADAS by
  ----------------

  Author : Martin O'Mullane
  Date   : 28/10/10

----------------------------------------------------------------------------

  Unphysical A values. Set A=1.0E-30 for following transitions :
     20    21    A =   4.47E-01
     24    25    A =   6.68E-08
     43    45    A =   4.39E-11
     43    49    A =   1.96E-10
     44    45    A =   1.04E-03
     44    49    A =   1.12E+01
     46    47    A =   1.17E-02
     46    49    A =   3.06E+01
     46    48    A =   3.38E-14
     40    49    A =   5.56E+01
     60    65    A =   6.56E-01
     61    65    A =   2.79E+00
     62    65    A =   5.42E-03
     63    65    A =   8.67E-02
     70    72    A =   8.37E-01
     71    72    A =   9.56E-02

-------------------------------------------------------------------------------

 Level list :

     1   2   3   4   5   6   7   8   9  10
    11  12  13  14  15  16  17  18  19  20
    21  22  23  24  25  26  27  28  29  30
    31  32  33  34  35  36  37  38  39  40
    41  42  43  44  45  46  47  48  49  50
    51  52  53  54  55  56  57  58  59  60
    61  62  63  64  65  66  67  68  69  70
    71  72  73  74  75  76  77  78  79  80
    81  82  83  84  85  86

 Original level order :

     1   2   3   4   5   6   7   8   9  10
    11  12  13  14  15  16  17  18  19  21
    23  25  20  22  24  26  27  28  29  31
    30  32  33  34  36  35  37  39  38  45
    47  49  40  41  42  43  44  48  46  50
    51  52  53  54  55  56  57  65  58  59
    60  61  62  64  63  66  67  68  72  69
    70  71  73  74  75  76  77  78  79  80
    81  83  82  84  85  86

-------------------------------------------------------------------------------

 Filtered adf04 file to 
  - sort energy levels 
  - remove non physical A values from
    energy level reversals
  - remove energies above ionisation potential
  - remove duplicate transitions

 Code     : ADAS utility program, filter04
 Date     : 28-10-2010
 Producer : Martin O'Mullane              

-------------------------------------------------------------------------------

 Regenerated to use the standard ADAS temperature set.

 Add the transitions in the CHIANTI source which have a transition
 probability but no accompanying effective collision strength and
 set these upsilons to zero.

 Update : Martin O'Mullane
 Date   : 28-10-2010
-------------------------------------------------------------------------------

Contributors

  • CHIANTI
  • Martin O'Mullane
  • Processes
  • States
  • Comments
  • Origins

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