chv6_ic#fe25.dat

• Spontaneous Emission: Fe⁺²⁵(i) → Fe⁺²⁵(j) + hv
• Electron Impact Excitation: Fe⁺²⁵(i) + e → Fe⁺²⁵(j) + e

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  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %observed energy levels: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995, NIST Database
       for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61
   %theoretical energy levels:  Ballance, C.P., Badnell, N.R., Berrington, K.A., 2002, J.Phys.B, 35, 1095
   %comment: ionization limit is 74829600
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   K.P. Dere - July 21, 2005

  A-values levels :
   %filename: fe_26.wgfa
   %observed energy levels: Martin,W.C., Sugar,J., Musgrove,A., Dalton,G.R., 1995,
       NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61.
   % A values: Parpia,F.A., Johnson,W.R., 1982, Phys. Rev. A, 26, 1142.
   %oscillator strengths: Wiese,W.L., Smith,M.W., Glennon,B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4.
   %comment: Wiese's f values are  hydrogenic
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Ken Dere 1998

  Collision strengths :

   %filename: fe_26.splups
   %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4
   %effective collision strengths: Ballance, C.P., Badnell, N.R., Berrington, K.A., 2002, J.Phys.B, 35, 1095
   %comment: effective collision strengths were provided in the temperature range 6.0 < Log T < 8.5
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   K.P.Dere - May 15, 2002



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

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

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 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

 Original level order :

     1   3   2   4   6   5   8   7   9  11
    10  13  12  15  14  16  18  17  20  19
    22  21  24  23  25

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 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              

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 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
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Contributors

• CHIANTI
• Nigel Badnell
• Connor Ballance
• Keith Berrington
• K P Dere
• Martin O'Mullane