chv6_ic#ca10.dat

• Spontaneous Emission: Ca⁺¹⁰(i) → Ca⁺¹⁰(j) + hv
• Electron Impact Excitation: Ca⁺¹⁰(i) + e → Ca⁺¹⁰(j) + e

A+10        20        11       4502441.2
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  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %energy levels (3,5,17,23,27,31,33,35,37,55,70): Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R.,
       1999, NIST Database for Atomic Spectroscopy, Version 2.0, NIST Standard Reference Database 61.
   %energy levels (4,7-10,13,14,19-22,24-26,44,52): Crance,M., 1973, Atomic Data, 5, 185
   %energy levels (59,60): Fawcett,B.C., Bromage,G.E., Hayes,R.W., 1979, MNRAS, 186, 113
   %energy levels (11,50,53,54,58,62): Kastner,S.O., Behring, W.E., Cohen,L., 1975, ApJ, 199, 777
   %Theoretical energy levels: Zhang, H. et al., ADNDT, 1987, 37, 17
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi 2000

  A-values levels :
   %filename: ca_11.wgfa
   %observed energy levels (3,5,17,23,27,31,33,35,37,55,70): Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R.,
       1999, NIST Database for Atomic Spectroscopy, Version 2.0, NIST Standard Reference Database 61
   %observed energy levels (4,7-10,13,14,19-22,24-26,44,52): Crance, M., 1973, Atomic Data, 5, 185
   %observed energy levels (59,60): Fawcett, B.C., Bromage, G.E., Hayes, R.W., 1979, MNRAS, 186, 113
   %observed energy levels (11,50,53,54,58,62): Kastner, S.O., Behring, W.E., Cohen, L., 1975, ApJ, 199, 777
   %theoretical energy levels: Zhang, H. et al., ADNDT, 1987, 37, 17
   %oscillator strengths transitions involving the ground level: Zhang, H. et al., ADNDT, 1987, 37, 17
   %oscillator strengths transitions among the 2p53l configurations: Hibbert, Le Dourneuf, Mohan, ADNDT, 1993, 53, 23
   % All other radiative data: SSTRUCT calculation, with a 15 configuration model including:

               2s2.2p6,
               2s2.2p5{3s, 3p, 3d}, 2s.2p6{3s, 3p, 3d}
               2s2.2p5{4s, 4p, 4d, 4f}, 2s.2p6{4s, 4p, 4d, 4f}

   %comment: SSTRUCT radiative data have been corrected for the differences between experimental
             and theoretical energy levels, where possible.
   %comment: negative wavelengths have been computed using theoretical energy levels.
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi 2000

  Collision strengths :

   %filename: ca_11.splups
   %oscillator strengths transitions involving the ground level: Zhang, H. et al., ADNDT, 1987, 37, 17
   %oscillator strengths transitions among the 2p53l configurations: Hibbert, Le Dourneuf, Mohan, ADNDT, 1993, 53, 23
   % All other oscillator strengths: SSTRUCT calculation, with a 15 configuration model (see file ca_11.wgfa)
   %collision strengths: Zhang, H. et al., ADNDT, 1987, 37, 17
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi 2000



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

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

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

 The following levels were above the ionisation potential :    4502441.2

     78 2s.2p6.4p 3P0      (3)1( 0.0)       4546407.0
     79 2s.2p6.4p 3P1      (3)1( 1.0)       4546908.0
     80 2s.2p6.4p 3P2      (3)1( 2.0)       4548506.0
     81 2s.2p6.4p 1P1      (1)1( 1.0)       4551807.0
     82 2s.2p6.4d 3D1      (3)2( 1.0)       4630677.0
     83 2s.2p6.4d 3D2      (3)2( 2.0)       4630809.0
     84 2s.2p6.4d 3D3      (3)2( 3.0)       4631011.0
     85 2s.2p6.4d 1D2      (1)2( 2.0)       4638376.0
     86 2s.2p6.4f 3F2      (3)3( 2.0)       4662202.0
     87 2s.2p6.4f 3F3      (3)3( 3.0)       4662308.0
     88 2s.2p6.4f 3F4      (3)3( 4.0)       4662404.0
     89 2s.2p6.4f 1F3      (1)3( 3.0)       4662808.0

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

 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  87  88  89

 Original level order :

     1   2   3   4   5   6   7   8  10   9
    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  58  56  57  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  87  88  89

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

 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
• Hong Zhang
• Martin O'Mullane