chv6_ic#ca4.dat

Resolved Specific Ion Data Collections

Ion
Ca4+
Temperature Range
1.077 eV → 1077 eV

ADF04

Filename
chv6_ic#ca4.dat
Full Path
adf04/copch#20/chv6_ic#ca4.dat
Download data
  • Spontaneous Emission: Ca+4(i) → Ca+4(j) + hv
  • Electron Impact Excitation: Ca+4(i) + e → Ca+4(j) + e
3s2.3p4 3p2 3P2.0 0.0 cm-1
3s2.3p4 3p1 3P1.0 0.0 cm-1
3s2.3p4 3p0 3P0.0 0.0 cm-1
3s2.3p4 1d2 1D2.0 18963.0 cm-1
3s2.3p4 1s0 1S0.0 42754.0 cm-1
A+ 4        20         5        741265.4
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  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %Observed energies: v.3.0.3 of the online NIST database
   %theoretical energies: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347
   %comment: The theoretical energies are from Table 3 of Galavis et al. and are for LS states.
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   Peter Young   -   9-Jun-2006

  A-values levels :
   %filename: ca_5.wgfa
   %Observed energies: v.3.0.3 of the online NIST database
   %A-values: Biemont, E., & Hansen, J.E., 1986, Phys. Scripta, 34, 116
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   Peter Young   -   9-Jun-2006

  Collision strengths :

   %filename: ca_5.splups
   %Theoretical energies: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347
   %Upsilons: Galavis, M.E., Mendoza, C., Zeippen, C.J. 1995, A&ASS 111, 347
   %comment: Observed energies used for transitions between levels 1,2 and 3.
   %comment: The original upsilons are valid over the range 10^3 - 10^5 K.  The spline fits reproduce the original upsilons to within 0.38%.
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %    Peter Young  -   9-Jun-2006



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

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

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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
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Contributors

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

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