chv6_ic#fe25.dat

Resolved Specific Ion Data Collections

Ion
Fe25+
Temperature Range
29.12 eV → 2.912 x 104 eV

ADF04

Filename
chv6_ic#fe25.dat
Full Path
adf04/copch#26/chv6_ic#fe25.dat
Download data
  • Spontaneous Emission: Fe+25(i) → Fe+25(j) + hv
  • Electron Impact Excitation: Fe+25(i) + e → Fe+25(j) + e
1s 2s1/2 2S0.5 0.0 cm-1
2p 2p1/2 2P0.5 56099100.0 cm-1
2s 2s1/2 2S0.5 56100200.0 cm-1
2p 2p3/2 2P1.5 56266000.0 cm-1
3p 2p1/2 2P0.5 66537300.0 cm-1
3s 2s1/2 2S0.5 66538600.0 cm-1
3d 2d3/2 2D1.5 66586700.0 cm-1
3p 2p3/2 2P1.5 66586800.0 cm-1
3d 2d5/2 2D2.5 66603100.0 cm-1
4p 2p1/2 2P0.5 70183800.0 cm-1
4s 2s1/2 2S0.5 70184700.0 cm-1
4d 2d3/2 2D1.5 70204500.0 cm-1
4p 2p3/2 2P1.5 70204700.0 cm-1
4f 2f5/2 2F2.5 70211400.0 cm-1
4d 2d5/2 2D2.5 70211400.0 cm-1
4f 2f7/2 2F3.5 70214900.0 cm-1
5p 2p1/2 2P0.5 71868700.0 cm-1
5s 2s1/2 2S0.5 71869400.0 cm-1
5d 2d3/2 2D1.5 71879200.0 cm-1
5p 2p3/2 2P1.5 71879400.0 cm-1
5f 2f5/2 2F2.5 71882700.0 cm-1
5d 2d5/2 2D2.5 71882700.0 cm-1
5g 2g7/2 2G3.5 71884500.0 cm-1
5f 2f7/2 2F3.5 71884500.0 cm-1
5g 2g9/2 2G4.5 71885500.0 cm-1
----------------------------------------------------------------------------

  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

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

 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

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

 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
  • Nigel Badnell
  • Connor Ballance
  • Keith Berrington
  • Martin O'Mullane
  • Processes
  • States
  • Comments
  • Origins

Data Classes