chv6_ic#fe7.dat

• Spontaneous Emission: Fe⁺⁷(i) → Fe⁺⁷(j) + hv
• Electron Impact Excitation: Fe⁺⁷(i) + e → Fe⁺⁷(j) + e

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  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %Experimental energy levels: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1999,
       NIST Database for Atomic Spectroscopy, Version 2.0, NIST Standard Reference Database 61
   %Experimental energy levels (3p6.4d levels - 51,52): Ekberg, J.O. & Feldman U., 2003, ApJ, 595, 517
   %Experimental energy levels (3,4,5,6,35,36,40): Landi, E. & Young, P.R., 2009, ApJ, submitted
   %theoretical energy levels: Griffin, D.C., Pindzola, M.S., Badnell, N.R., 2000, A&ASS, 142, 317
   %theoretical energy levels n=5,6,7: Czyzak,S.J., Krueger,T.K., 1966, ApJ, 144, 381
   %Comment: Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8 report
             an inversion of energies between levels 70 and 72 (same J). For consistency with Griffin
             et al 2000, who adapted their atomic structure calculation to a set of observed energies
             identical to the NIST one, we use the NIST v.2 level ordering.

             The energies for 3p5.3d2 4DJ (levels 3-6) have been updated using the
             lines observed between 253.9 and 255.8 angstroms in Hinode/EIS spectra.

             The energy for 3p5.3ds 2G7/2 (levels 40) has been updated using the
             line observed at 206.78 angstroms by Hinode/EIS. The theoretical
             splitting for the doublet has been used to update the theoretical
             energy for level 39 (2G9/2).
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E.Landi and P.R.Young  -   Nov 2008

  A-values levels :
   %filename: fe_8.wgfa
   %Experimental energy levels: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1999,
       NIST Database for Atomic Spectroscopy, Version 2.0, NIST Standard Reference Database 61
   %Experimental energy levels (3p6.4d levels - 51,52): Ekberg, J.O. & Feldman U., 2003, ApJ, 595, 517
   %Experimental energy levels (3,4,5,6,35,36,40): Landi, E. & Young, P.R., 2009, ApJ, submitted
   %theoretical energy levels: Griffin, D.C., Pindzola, M.S., Badnell, N.R., 2000, A&ASS, 142, 317
   %theoretical energy levels n=5,6,7: Czyzak,S.J., Krueger,T.K., 1966, ApJ, 144, 381
   %Comment: Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8 report
             an inversion of energies between levels 70 and 72 (ssame J). For consistency with Griffin
             et al 2000, who adapted their atomic structure calculation to a set of observed energies
             identical to the NIST v.2 one, we use the NIST v.2 level ordering.
   %Radiative data: Griffin, D.C., Pindzola, M.S., Badnell, N.R., 2000, A&ASS, 142, 317
   %Radiative data n=5,6,7: Czyzak,S.J., Krueger,T.K., 1966, ApJ, 144, 381
   %Radiative data 1 - 2 transition: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1999,
         NIST Database for Atomic Spectroscopy, Version 2.0, NIST Standard Reference Database 61
   %Radiative data for levels with J=9/2, 11/2: calculated using SUPERSTRUCTURE, with the configurations
                  3s2.3p6.3d, 3s2.3p5.3d2, 3s2.3p5.3d.4s, 3s2.3p6.4s, 3s2.3p6.4p, 3s2.3p6.4d, 3s2.3p6.4f,
                  3s2.3p4.3d3, 3s2.3p3.3d4
   %comment: SUPERSTRUCTURE radiative data have been corrected for the differences between experimental
             and SUPERSTRUCTURE transition wavelength differences, where experimental values were available.
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E.Landi and P.R.Young   -   Nov 2008

  Collision strengths :

   %filename: fe_8.splups
   %Oscillator strengths: Griffin, D.C., Pindzola, M.S., Badnell, N.R., 2000, A&ASS, 142, 317
   %Effective collision strengths: Griffin, D.C., Pindzola, M.S., Badnell, N.R., 2000, A&ASS, 142, 317
   %collision strengths and gf values n=5,6,7:  Czyzak,S.J., Krueger,T.K., 1966, ApJ, 144, 381
   %comment: effective collision strengths were provided in the temperature range 4.5 < Log T < 6.5
   %comment: added collisional data for transitions involving levels 21,25,28,29,39. They affect
             level populations at electron densities larger than 10^9 cm^-3 (June 2003).
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Enrico Landi - June 2003



  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  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

 Original level order :

     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  39  36  37  38  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  78  79  80  81  76
    77  82  83

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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.

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

Contributors

• CHIANTI
• Nigel Badnell
• Don Griffin
• Martin O'Mullane