chv6_ic#si8.dat

Resolved Specific Ion Data Collections

Ion
Si8+
Temperature Range
3.490 eV → 3490 eV

ADF04

Filename
chv6_ic#si8.dat
Full Path
adf04/copch#14/chv6_ic#si8.dat
Download data
  • Spontaneous Emission: Si+8(i) → Si+8(j) + hv
  • Electron Impact Excitation: Si+8(i) + e → Si+8(j) + e
2s2.2p2 3p0 3P0.0 0.0 cm-1
2s2.2p2 3p1 3P1.0 2567.0 cm-1
2s2.2p2 3p2 3P2.0 6458.0 cm-1
2s2.2p2 1d2 1D2.0 55598.0 cm-1
2s2.2p2 1s0 1S0.0 104063.0 cm-1
2s.2p3 5s2 5S2.0 138482.0 cm-1
2s.2p3 3d2 3D2.0 293060.0 cm-1
2s.2p3 3d1 3D1.0 293110.0 cm-1
2s.2p3 3d3 3D3.0 293353.0 cm-1
2s.2p3 3p0 3P0.0 344163.0 cm-1
2s.2p3 3p1 3P1.0 344269.0 cm-1
2s.2p3 3p2 3P2.0 344461.0 cm-1
2s.2p3 1d2 1D2.0 454782.0 cm-1
2s.2p3 3s1 3S1.0 461461.0 cm-1
2s.2p3 1p1 1P1.0 505953.0 cm-1
2p4 3p2 3P2.0 687200.0 cm-1
2p4 3p1 3P1.0 691715.0 cm-1
2p4 3p0 3P0.0 693621.0 cm-1
2p4 1d2 1D2.0 740179.0 cm-1
2p4 1s0 1S0.0 843432.0 cm-1
2s2.2p3s 3p0 3P0.0 1645070.0 cm-1
2s2.2p3s 3p1 3P1.0 1646720.0 cm-1
2s2.2p3s 3p2 3P2.0 1651730.0 cm-1
2s2.2p3s 1p1 1P1.0 1664790.0 cm-1
2s2.2p3p 1p1 1P1.0 1718770.0 cm-1
2s2.2p3p 3d1 3D1.0 1724600.0 cm-1
2s2.2p3p 3d2 3D2.0 1725920.0 cm-1
2s2.2p3p 3d3 3D3.0 1730230.0 cm-1
2s2.2p3p 3s1 3S1.0 1738090.0 cm-1
2s2.2p3p 3p0 3P0.0 1751940.0 cm-1
2s2.2p3p 3p1 3P1.0 1753920.0 cm-1
2s2.2p3p 3p2 3P2.0 1756190.0 cm-1
2s2.2p3p 1d2 1D2.0 1773180.0 cm-1
2s2.2p3p 1s0 1S0.0 1800520.0 cm-1
2s2.2p3d 3f2 3F2.0 1810730.0 cm-1
2s2.2p3d 3f3 3F3.0 1813920.0 cm-1
2s2.2p3d 1d2 1D2.0 1816280.0 cm-1
2s2.2p3d 3f4 3F4.0 1817430.0 cm-1
2s2.2p3d 3d1 3D1.0 1831770.0 cm-1
2s2.2p3d 3d2 3D2.0 1832480.0 cm-1
2s2.2p3d 3d3 3D3.0 1834890.0 cm-1
2s2.2p3d 3p2 3P2.0 1838390.0 cm-1
2s2.2p3d 3p1 3P1.0 1839400.0 cm-1
2s2.2p3d 3p0 3P0.0 1839920.0 cm-1
2s2.2p3d 1p1 1P1.0 1864210.0 cm-1
2s2.2p3d 1f3 1F3.0 1865340.0 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 (n=2): Edlen, B., 1985, Physica Scripta, 31, 345
   %energy levels (n=3): Martin, W.C., Sugar, J., Musgrove, A., Dalton, G.R., 1995,
      NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61
   %Theoretical energy levels: Bhatia, A.K., Doschek, G.A., 1993, ADNDT, 55, 281
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   E.Landi 2000

  A-values levels :
   %filename: si_9.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
   %Theoretical energy levels: Bhatia, A.K., Doschek, G.A., 1993, ADNDT, 55, 281
   %A-values (ground configuration): Galavis, M.E., Mendoza, C., Zeippen, C.J., 1997, A&AS, 123, 159
   %A values and oscillator strengths: Bhatia, A.K., Doschek, G.A., 1993, ADNDT, 55, 281
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   E.Landi and P.R. Young - 17-Jul-2006

  Collision strengths :

   %filename: si_9.splups
   %oscillator strengths: Bhatia, A.K., Doschek, G.A., 1993, ADNDT, 55, 281
   %collision strengths: Bhatia, A.K., Doschek, G.A., 1993, ADNDT, 55, 281
   %effective collision strengths (ground configuration): Aggarwal, K.M., 1983, J.Phys.B, 16, L59
   %comment: Relativistic effects are not included in the Aggarwal calculations, but he
      does a comparison with the DW calcs of Mason & Bhatia (MNRAS 184, 423,
      1978) and finds good agreement. A comparison with the more recent Iron
      Project data of Lennon & Burke (AAS 103, 273, 1994) also shows good
      agreement.
   %comment: As Aggarwal did not present calculated energies, observed values have been used.
   %comment: effective collision strengths were provided in the temperature range 5.5 < Log T < 6.4
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Enrico Landi and Peter Young, Nov 2002



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

  Author : Martin O'Mullane
  Date   : 12/03/13

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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     : 12-03-2013
 Producer : Martin O'Mullane              

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Contributors

  • CHIANTI
  • Kanti Aggarwal
  • Martin O'Mullane
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