chv6_ic#fe19.dat

• Spontaneous Emission: Fe⁺¹⁹(i) → Fe⁺¹⁹(j) + hv
• Electron Impact Excitation: Fe⁺¹⁹(i) + e → Fe⁺¹⁹(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 (2-5): Kucera et al., 2000, ApJ, 538, 424
   %Observed energy levels (6-15): Edlen, B., 1984,P ysicaS cripta, 30, 135
   %Observed energy levels (n=3): identifications from the X-ray line list by Landi &P hillips 2005, ApJS, 160, 286
   %Observed energy levels (n=4,5):S hirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8
   %Theoretical energy levels (levels up to n=4): Witthoeft, M.C.,D el Zanna,G ., & Badnell, N.R. 2007, A&A, 466, 763
   %Theoretical energy levels (n=5 levels): Landi &G u, 2006, ApJ, 640, 1171
   %Theoretical energy levels (above ionization): Bautista, M.A., Mendoza, C., Kallman, T.R.,P almeri, P., 2004, A&A, 418, 1171
   %comment: theoretical energy levels fromP almeri et al are treated as experimental ones when no measured value was available
   % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %  Giulio Del Zanna and Enrico Landi - Oct 2008

  A-values levels :
   %filename: fe_20.wgfa
   %Observed energy levels (2-5): Kucera et al., 2000, ApJ, 538, 424
   %Observed energy levels (6-15): Edlen, B., 1984, Pysica Scripta, 30, 135
   %Observed energy levels (n=3): identifications from the X-ray line list by Landi & Phillips 2005, ApJS, 160, 286
   %Observed energy levels (n=4,5): Shirai,T., Sugar,J., Musgrove,A., Wiese,W.L., 2000, J.Phys.Chem.Ref.Data, Monograph 8
   %Theoretical energy levels (levels up to n=4): Witthoeft, M.C., Del Zanna, G., & Badnell, N.R. 2007, A&A, 466, 763
   %Theoretical energy levels (n=5 levels): Landi & Gu, 2006, ApJ, 640, 1171
   %Theoretical energy levels (above ionization): Bautista, M.A., Mendoza, C., Kallman, T.R., Palmeri, P., 2004, A&A, 418, 1171
   %A and gf values (levels up to n=4): Witthoeft, M.C., Del Zanna, G., & Badnell, N.R. 2007, A&A, 466, 763
   %A and gf values (n=5 levels): Landi & Gu, 2006, ApJ, 640, 1171
   %Radiative data innershell transitions to levels 1 to 15: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175
   %Radiative data transitions to levels 360 and up: Bautista, M.A., Mendoza, C., Kallman, T.R., Palmeri, P., 2004, A&A, 418, 1171
   %Autoionization rates: Palmeri P., Mendoza C., Kallman T.R., Bautista M.A., 2003, A&A, 403, 1175
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %     Giulio Del Zanna and Enrico Landi - Oct 2008

  Collision strengths :

   %filename: fe_20.splups
   %oscillator strengths (up to n=4 levels): Witthoeft, M.C., Del Zanna, G., & Badnell, N.R. 2007, A&A, 466, 763
   %oscillator strengths (n=5 levels): Landi & Gu, 2006, ApJ, 640, 1171
   %oscillator strengths (above ionization): Bautista, M.A., Mendoza, C., Kallman, T.R., Palmeri, P., 2004, A&A, 418, 1171
   %effective collision strengths (up to n=4 levels): Witthoeft, M.C., Del Zanna, G., & Badnell, N.R. 2007, A&A, 466, 763
   %effective collision strengths (n=5 levels): Landi & Gu, 2006, ApJ, 640, 1171
   %effective collision strengths (above ionization): Bautista, M.A., Mendoza, C., Kallman, T.R., Palmeri, P., 2004, A&A, 418, 1171
   %comment: all excitations from the ground configuration have been retained form the original calculation.
   %comment: effective collision strengths from FAC were provided in the temperature range 1.16e6 < T < 5.8e7
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   %   Giulio Del Zanna - Oct 2008



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

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

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 The following levels were above the ionisation potential :   12708717.8

    360 1s.2s2.2p4 4P5/2      (4)1( 2.5)      52397474.0
    361 1s.2s2.2p4 4P3/2      (4)1( 1.5)      52473178.0
    362 1s.2s2.2p4 4P1/2      (4)1( 0.5)      52490173.0
    363 1s.2s2.2p4 2D3/2      (2)2( 1.5)      52615991.0
    364 1s.2s2.2p4 2D5/2      (2)2( 2.5)      52653071.0
    365 1s.2s2.2p4 2P1/2      (2)1( 0.5)      52695023.0
    366 1s.2s2.2p4 2P3/2      (2)1( 1.5)      52703105.0
    367 1s.2s2.2p4 2S1/2      (2)0( 0.5)      52825674.0
    368 1s.2s(3P).2p5 4P5/2   (4)1( 2.5)      53149964.0
    369 1s.2s(3P).2p5 4P3/2   (4)1( 1.5)      53210417.0
    370 1s.2s(3P).2p5 4P1/2   (4)1( 0.5)      53262867.0
    371 1s.2s(3P).2p5 2P3/2   (2)1( 1.5)      53447553.0
    372 1s.2s(3P).2p5 2P1/2   (2)1( 0.5)      53483009.0
    373 1s.2s(1P).2p5 2P3/2   (2)1( 1.5)      53604825.0
    374 1s.2s(1P).2p5 2P1/2   (2)1( 0.5)      53653195.0
    375 1s.2p6 2S1/2          (2)0( 0.5)      54362980.0

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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              

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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
• Nigel Badnell
• Mike Witthoeft
• Manuel Bautista
• Martin O'Mullane