ls#ni15.dat

Resolved Specific Ion Data Collections

Ion
Ni15+
Temperature Range
22.06 eV → 4412 eV

ADF04

Filename
ls#ni15.dat
Full Path
adf04/copmm#28/ls#ni15.dat
Download data
  • Spontaneous Emission: Ni+15(i) → Ni+15(j) + hv
  • Electron Impact Excitation: Ni+15(i) + e → Ni+15(j) + e
24515 2P2.5 0.0 cm-1
14525 4P5.5 256778.0 cm-1
14525 2D4.5 339911.0 cm-1
14525 2S0.5 387897.0 cm-1
14525 2P2.5 438937.0 cm-1
24516 2D4.5 521160.0 cm-1
35 4S1.5 663312.0 cm-1
35 2D4.5 677135.0 cm-1
14515516 4F13.5 730324.0 cm-1
35 2P2.5 737775.0 cm-1
14515516 4P5.5 775365.0 cm-1
14515516 4D9.5 780716.0 cm-1
14515516 2D4.5 796438.0 cm-1
14515516 2F6.5 839510.0 cm-1
14515516 2P2.5 881981.0 cm-1
14515516 2F6.5 914539.0 cm-1
14515516 2D4.5 928489.0 cm-1
14515516 2P2.5 936073.0 cm-1
14526 4F13.5 1269270.0 cm-1
14526 4P5.5 1298280.0 cm-1
14526 2D4.5 1318460.0 cm-1
14526 2G8.5 1329470.0 cm-1
14526 2F6.5 1339610.0 cm-1
14526 2P2.5 1366790.0 cm-1
14526 2S0.5 1391950.0 cm-1
36 4F13.5 2097890.0 cm-1
36 4P5.5 2125480.0 cm-1
36 2G8.5 2127250.0 cm-1
36 2H10.5 2137160.0 cm-1
36 2D4.5 2140010.0 cm-1
36 2P2.5 2141950.0 cm-1
36 2F6.5 2165150.0 cm-1
36 2D4.5 2203740.0 cm-1
---------------------------------------------------------------------------------

     Generated from Cowan Atomic Structure Program

     M O'Mullane        18:22  19/05/1994



     SCF method used                      : HR

     Scale factors for Slater Parameters  : 80 99 85 85 60

     Optically allowed transitions        : yes

     Optically forbidden transitions M1   : parity 1

     Optically forbidden transitions E2   : parity 1

     Born Collision-Strength  - print     :  9

                              - forbidden :  0 -> 2

                              - allowed   :  1 -> 1

                              - included  :  3,all

     Parity 1    Parity 2    Allowed
          394           0        841     initially
           79           0        237     reduced

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

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

   Martin O'Mullane
   29-11-2011

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

Contributors

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

Data Classes