chv6_ic#mg3.dat

• Spontaneous Emission: Mg⁺³(i) → Mg⁺³(j) + hv
• Electron Impact Excitation: Mg⁺³(i) + e → Mg⁺³(j) + e

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

  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %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.
   %energy levels: Bhatia, A.K., private communications
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Enrico Landi 2002

  A-values levels :
   %filename: mg_4.wgfa
   %energy levels: Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995,
       NIST Standard Reference Database 61, NIST Database for Atomic Spectroscopy, Version 1.0
   %transition probabilities (1-2): Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995,
       NIST Standard Reference Database 61, NIST Database for Atomic Spectroscopy, Version 1.0
   %transition probabilities: Blackford, H.M.S., Hibbert, A., 1994, ADNDT, 58, 101
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %  K.P. Dere 1995

  Collision strengths :

   %filename: mg_4.splups
   %oscillator strengths: Blackford, H.M.S., Hibbert, A., 1994, ADNDT, 58, 101
   %effective collision strengths: Saraph, H.E., Tully, J.A., 1994, A&AS, 107, 29
   %collision strengths: Mohan, M., Baluja, K.L., Hibbert, A., 1988, Phys. Scripta, 38, 699
   %comment: effective collision strengths were provided in the temperature range 3.0 < Log T < 5.25
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %  K.P. Dere 1994



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

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

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

 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.

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

Contributors

• CHIANTI
• K P Dere
• Martin O'Mullane