chv6_ic#mg9.dat

Resolved Specific Ion Data Collections

Ion
Mg9+
Temperature Range
4.308 eV → 4308 eV

ADF04

Filename
chv6_ic#mg9.dat
Full Path
adf04/copch#12/chv6_ic#mg9.dat
Download data
  • Spontaneous Emission: Mg+9(i) → Mg+9(j) + hv
  • Electron Impact Excitation: Mg+9(i) + e → Mg+9(j) + e
1s2.2s 2s1/2 2S0.5 0.0 cm-1
1s2.2p 2p1/2 2P0.5 160002.0 cm-1
1s2.2p 2p3/2 2P1.5 163978.0 cm-1
1s2.3s 2s1/2 2S0.5 1682940.0 cm-1
1s2.3p 2p1/2 2P0.5 1726970.0 cm-1
1s2.3p 2p3/2 2P1.5 1728180.0 cm-1
1s2.3d 2d3/2 2D1.5 1744230.0 cm-1
1s2.3d 2d5/2 2D2.5 1744560.0 cm-1
1s2.4s 2s1/2 2S0.5 2252600.0 cm-1
1s2.4p 2p1/2 2P0.5 2270660.0 cm-1
1s2.4p 2p3/2 2P1.5 2271230.0 cm-1
1s2.4d 2d3/2 2D1.5 2278000.0 cm-1
1s2.4d 2d5/2 2D2.5 2278160.0 cm-1
1s2.4f 2f5/2 2F2.5 2279210.0 cm-1
1s2.4f 2f7/2 2F3.5 2279290.0 cm-1
1s2.5s 2s1/2 2S0.5 2512060.0 cm-1
1s2.5p 2p1/2 2P0.5 2521180.0 cm-1
1s2.5p 2p3/2 2P1.5 2521420.0 cm-1
1s2.5d 2d3/2 2D1.5 2524970.0 cm-1
1s2.5d 2d5/2 2D2.5 2525050.0 cm-1
1s2.5f 2f5/2 2F2.5 2525530.0 cm-1
1s2.5f 2f7/2 2F3.5 2525610.0 cm-1
1s2.5g 2g7/2 2G3.5 2526020.0 cm-1
1s2.5g 2g9/2 2G4.5 2526100.0 cm-1
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  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %energy levels (1-24): Martin, W.C., Zalubas, R., 1980, J.Phys.Chem.Ref.Data, 9, 1.
   %Theoretical energy levels (1-24): Zhang,H.L., Sampson,D.H., Fontes,C.J., ADNDT, 44, 31.
   %Innershell energy levels: Fuhr et al, 1999, NIST Atomic Spectra Database Version 2.0
   %Innershell theoretical energy levels: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E. Landi - July 1999

  A-values levels :
   %filename: mg_10.wgfa
   %observed energy levels: Martin,W.C., Zalubas,R., 1980, J.Phys.Chem.Ref.Data, 9, 1.
   % Theoretical energy levels: Zhang,H.L., Sampson,D.H., Fontes,C.J., 1990, ADNDT, 44, 31.
   %oscillator strengths: H.L. Zhang, D.H. Sampson, C.J. Fontes, 1990, ADNDT, 44, 31
   %oscillator strengths: Martin, I., Karwowski, J., Diercksen, G.H.F., Barrientos, C., 1993, A&AS, 100, 595.
   % Innershell radiative data: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
   %Comment: Other radiative data were calculated using SUPERSTRUCTURE with a 23 configuration model
   %A values (autoionizing): Vainshtein, L.A., Safronova, U.I., 1978, ADNDT, 21, 49-68.
      and 1980, ADNDT, 25, 311 - updated by U.I. Safronova, 1999
   %comment: unobserved lines
       2   25        -9.5974      7.530e-03      2.725e+11   1s2.(1S).2p 2P0.5 -         1s.2s2 2S0.5
       3   25        -9.6010      1.401e-02      5.066e+11   1s2.(1S).2p 2P1.5 -         1s.2s2 2S0.5
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   E. Landi and K.P. Dere - Nov 1999

  Collision strengths :

   %filename: mg_10.splups
   %oscillator strengths: Zhang, Sampson, Fontes, 1990, ADNDT, 44, 31
   %collision strengths: Zhang, Sampson, Fontes, 1990, ADNDT, 44, 31
   %oscillator strengths innershell transitions: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
   %collision strengths innershell transitions: Goett, S.J., Sampson, D.H., 1983, ADNDT, 29, 535
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % E.Landi and K.P.Dere - July 1999



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

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

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 The following levels were above the ionisation potential :    2964230.8

     25 1s.2s2 2S1/2       (2)0( 0.5)      10579555.0
     26 1s2s(3P).2p 4P1/2  (4)1( 0.5)      10619061.0
     27 1s2s(3P).2p 4P3/2  (4)1( 1.5)      10622221.0
     28 1s2s(3P).2p 4P5/2  (4)1( 2.5)      10625381.0
     29 1s2s(3P).2p 2P1/2  (2)1( 0.5)      10772341.0
     30 1s2s(3P).2p 2P3/2  (2)1( 1.5)      10775500.0
     31 1s.2p2 4P1/2       (4)1( 0.5)      10805525.0
     32 1s.2p2 4P3/2       (4)1( 1.5)      10808687.0
     33 1s.2p2 4P5/2       (4)1( 2.5)      10813427.0
     34 1s2s(1P).2p 2P1/2  (2)1( 0.5)      10830810.0
     35 1s2s(1P).2p 2P3/2  (2)1( 1.5)      10832389.0
     36 1s.2p2 2D3/2       (2)2( 1.5)      10911401.0
     37 1s.2p2 2D5/2       (2)2( 2.5)      10911401.0
     38 1s.2p2 2P1/2       (2)1( 0.5)      10941424.0
     39 1s.2p2 2P3/2       (2)1( 1.5)      10947745.0
     40 1s.2p2 2S1/2       (2)0( 0.5)      11037818.0

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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              

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

 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
  • Hong Zhang
  • Douglas Sampson
  • Martin O'Mullane
  • Processes
  • States
  • Comments
  • Origins

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