ls#kr9.dat

Resolved Specific Ion Data Collections

Ion
Kr9+
Temperature Range
8.617 eV → 1723 eV

ADF04

Filename
ls#kr9.dat
Full Path
adf04/copmm#36/ls#kr9.dat
Download data
  • Spontaneous Emission: Kr+9(i) → Kr+9(j) + hv
  • Electron Impact Excitation: Kr+9(i) + e → Kr+9(j) + e
65596 2D4.5 0.0 cm-1
65586518 4D9.5 950230.0 cm-1
65586518 4G17.5 957960.0 cm-1
65586518 2G8.5 957970.0 cm-1
65586518 2D4.5 963960.0 cm-1
65586518 4F13.5 966540.0 cm-1
65586518 2F6.5 968050.0 cm-1
65586518 4P5.5 984130.0 cm-1
65586518 2F6.5 986780.0 cm-1
65586518 2D4.5 993150.0 cm-1
65586518 2P2.5 998460.0 cm-1
65586518 4D9.5 1001700.0 cm-1
65586518 2H10.5 1003500.0 cm-1
65586518 2F6.5 1004800.0 cm-1
65586518 2D4.5 1007300.0 cm-1
65586518 2P2.5 1011100.0 cm-1
65586518 4S1.5 1013500.0 cm-1
65586518 2S0.5 1014200.0 cm-1
55606 2P2.5 1015600.0 cm-1
65586518 2G8.5 1021200.0 cm-1
65586518 2P2.5 1083100.0 cm-1
---------------------------------------------------------------------------------

     Generated from Cowan Atomic Structure Program

     M O'Mullane        16:18  19/10/1994



     SCF method used                      : HR

     Scale factors for Slater Parameters  : 95 99 85 85 60

     Optically allowed transitions        : yes

     Optically forbidden transitions M1   : both

     Optically forbidden transitions E2   : both

     Born Collision-Strength  - print     :  9

                              - forbidden :  0 -> 2

                              - allowed   :  1 -> 1

                              - included  :  1,all

     Parity 1    Parity 2    Allowed
            0           0         63     initially
            0           0         19     reduced

---------------------------------------------------------------------------------
   
   Level 19 had an incorrect Eissner label.

   Correct the orbital energy line to insert 0.0 for orbitals not present
   in the set of configurations.

   Martin O'Mullane
   29-11-2011

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Contributors

  • Martin O'Mullane
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