chv6_ic#mg10.dat

• Spontaneous Emission: Mg⁺¹⁰(i) → Mg⁺¹⁰(j) + hv
• Electron Impact Excitation: Mg⁺¹⁰(i) + e → Mg⁺¹⁰(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.
   %observed energy levels (2s2p 3P): Chen, M.H., Cheng, K.T., Johnson, W.R., 1993, Ph.Rev.A, 47, 3692
   %theoretical energy levels: Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % K.P.Dere and E.Landi 2000

  A-values levels :
   %filename: mg_11.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
   %observed energy levels (2s2p 3P): Chen, M.H., Cheng, K.T., Johnson, W.R., 1993, Ph.Rev.A, 47, 3692
   %theoretical energy levels: Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467
   %A values (1-2): Stefanelli, G.S., Beiersdorfer, P., Decaux, V., Widmann, K., 1995, Phys. Rev. A, 52, 3651
   %A values (1-3, 2-phot): Drake, G.W.F., Phys Rev A, 1986, 34, 2871
   %A values (1-5): Armour, I.A., Silver, J.D., Traebert, E., 1981, J. Phys. B, 14 ,3563
   %A values (1-6): Lin, C.D., Johnson, W.R., Dalgarno, A., Phys Rev A, 1977, 15, 154
   %A values (n=2,n=3): Porquet, D. & Dubau, J. 2000, A&AS, 143, 495
   %oscillator strengths and A values (1-23,37): Wiese, W.L., Fuhr, J.R., 1995,
      NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61
   %oscillator strengths (for transitions involving lower levels 1,2,3 not included in Porquet & Dubau):
      Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467,  Hydrogenic values
   %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4.
   %Comment: Wiese's oscillator strengths are hydrogenic
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % K.P.Dere and E.Landi - Aug 2006

  Collision strengths :

   %filename: mg_11.splups
   %oscillator strengths and A values (1-7,13,23,37): Wiese, W.L., Fuhr, J.R., 1995,
      NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61
   %oscillator strengths (for transitions involving lower levels 1,2,3):
      Sampson, D.H., Goett, S.J., Clark, R.E.H., 1983, ADNDT, 29, 467,  Hydrogenic values
   %oscillator strengths: Wiese, W.L., Smith, M.W., Glennon, B.M., 1966, Atomic Transition Probabilities, NSRDS-NBS-4 (hydrogenic)
   %effective collision strengths (levels 1-7): Zhang, H., Sampson, D.H., 1987, ApJSS, 63, 487
   %collison strengths: Sampson, D.H., Goett, S.J., Clark, R.E.H. 1983, ADNDT, 29, 467,  Hydrogenic values
   %comment: effective collision strengths were provided in the temperature range 5.8 < Log T < 7.25
   %produced as part of the Arcetri/Cambridge/NRL atomic 'CHIANTI' data base collaboration
   %
   % K.P.Dere and E. Landi 1998



  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

 Original level order :

     1   2   4   5   6   3   7   8  10  11
     9  12  14  15  16  17  13  18  19  20
    21  22  29  24  25  26  28  27  30  31
    23  32  33  34  35  36  49  38  39  40
    41  42  43  44  45  46  47  48  37

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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
• Douglas Sampson
• K P Dere
• Hong Zhang
• Martin O'Mullane