chv6_ic#ca7.dat

Resolved Specific Ion Data Collections

Ion
Ca7+
Temperature Range
2.757 eV → 2757 eV

ADF04

Filename
chv6_ic#ca7.dat
Full Path
adf04/copch#20/chv6_ic#ca7.dat
Download data
  • Spontaneous Emission: Ca+7(i) → Ca+7(j) + hv
  • Electron Impact Excitation: Ca+7(i) + e → Ca+7(j) + e
3s2.3p 2p1/2 2P0.5 0.0 cm-1
3s2.3p 2p3/2 2P1.5 4307.0 cm-1
3s.3p2 4p1/2 4P0.5 129823.0 cm-1
3s.3p2 4p3/2 4P1.5 131403.0 cm-1
3s.3p2 4p5/2 4P2.5 133764.0 cm-1
3s.3p2 2d3/2 2D1.5 171576.0 cm-1
3s.3p2 2d5/2 2D2.5 171832.0 cm-1
3s.3p2 2s1/2 2S0.5 216587.0 cm-1
3s.3p2 2p1/2 2P0.5 231016.0 cm-1
3s.3p2 2p3/2 2P1.5 233592.0 cm-1
3s2.3d 2d3/2 2D1.5 282353.0 cm-1
3s2.3d 2d5/2 2D2.5 282574.0 cm-1
3p3 2d3/2 2D1.5 335852.0 cm-1
3p3 2d5/2 2D2.5 336305.0 cm-1
3p3 4s3/2 4S1.5 345995.0 cm-1
3p3 2p1/2 2P0.5 377110.0 cm-1
3p3 2p3/2 2P1.5 377238.0 cm-1
3s.3p(3p).3d 4f3/2 4F1.5 377458.0 cm-1
3s.3p(3p).3d 4f5/2 4F2.5 378352.0 cm-1
3s.3p(3p).3d 4f7/2 4F3.5 379626.0 cm-1
3s.3p(3p).3d 4f9/2 4F4.5 381330.0 cm-1
3s.3p(3p).3d 4p5/2 4P2.5 408960.0 cm-1
3s.3p(3p).3d 4p3/2 4P1.5 409998.0 cm-1
3s.3p(3p).3d 4d1/2 4D0.5 410954.0 cm-1
3s.3p(3p).3d 4p1/2 4P0.5 412562.0 cm-1
3s.3p(3p).3d 4d3/2 4D1.5 413120.0 cm-1
3s.3p(3p).3d 4d5/2 4D2.5 413497.0 cm-1
3s.3p(3p).3d 4d7/2 4D3.5 413609.0 cm-1
3s.3p(3p).3d 2d3/2 2D1.5 423606.0 cm-1
3s.3p(3p).3d 2d5/2 2D2.5 423613.0 cm-1
3s.3p(3p).3d 2f5/2 2F2.5 444046.0 cm-1
3s.3p(3p).3d 2f7/2 2F3.5 447460.0 cm-1
3s.3p(3p).3d 2p3/2 2P1.5 483902.0 cm-1
3s.3p(3p).3d 2p1/2 2P0.5 485292.0 cm-1
3s.3p(1p).3d 2f7/2 2F3.5 486202.0 cm-1
3s.3p(1p).3d 2f5/2 2F2.5 487081.0 cm-1
3s.3p(1p).3d 2p1/2 2P0.5 501967.0 cm-1
3s.3p(1p).3d 2p3/2 2P1.5 502198.0 cm-1
3s.3p(1p).3d 2d3/2 2D1.5 506070.0 cm-1
3s.3p(1p).3d 2d5/2 2D2.5 506657.0 cm-1
A+ 7        20         8       1261522.4
----------------------------------------------------------------------------

  Data generated from CHIANTI version 6.0

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

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

  Energy levels :
   %observed energy levels: Churilov S.S., Levashov V.E., 1993, Physica Scripta 48, 425
   %theoretical energy levels: Churilov S.S., Levashov V.E., 1993, Physica Scripta 48, 425
   %comment: Churilov et al. experimental energies have been used to calculate A values from
             line strengths, so they are reported instead of the theoretical energies
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Enrico Landi - Aug 2001

  A-values levels :
   %filename: ca_8.wgfa
   %observed energy levels: Churilov S.S., Levashov V.E., 1993, Physica Scripta 48, 425
   %Radiative data: Landi, Storey & Zeippen 2004, ApJ, 607, 640
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Enrico Landi - Sept 2001

  Collision strengths :

   %filename: ca_8.splups
   %oscillator strengths: Landi, Storey, & Zeippen, 2004, ApJ, 607, 640
   %effective collision strengths: Landi, Storey & Zeippen, 2004, ApJ, 607, 640
   %Comment: upsilon have been fitted in the range 4.5 < Log T < 7.0
   %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration
   %
   % Enrico Landi - Sept 2001



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

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

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

 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

 Original level order :

     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  30  29
    31  32  33  34  35  36  37  38  39  40

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

 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
  • Martin O'Mullane
  • Processes
  • States
  • Comments
  • Origins

Data Classes