ls#f5.dat

Resolved Specific Ion Data Collections

Ion
F5+
Temperature Range
3.102 eV → 620 eV

ADF04

Filename
ls#f5.dat
Full Path
adf04/copmm#9/ls#f5.dat
Download data
  • Spontaneous Emission: F+5(i) → F+5(j) + hv
  • Electron Impact Excitation: F+5(i) + e → F+5(j) + e
21522 1S0.0 0.0 cm-1
21512513 3P4.0 90577.6 cm-1
21512513 1P1.0 172140.0 cm-1
21523 3P4.0 243643.0 cm-1
21523 1D2.0 268414.0 cm-1
21523 1S0.0 319235.0 cm-1
21512514 3S1.0 739799.0 cm-1
21512514 1S0.0 755502.0 cm-1
21512515 3P4.0 782961.0 cm-1
21512515 1P1.0 788859.0 cm-1
21512516 3D7.0 803894.0 cm-1
21512516 1D2.0 817122.0 cm-1
21513515 1P1.0 887143.0 cm-1
21513515 3D7.0 891232.0 cm-1
21513515 3S1.0 896761.0 cm-1
21513515 3P4.0 906835.0 cm-1
21513515 1D2.0 916195.0 cm-1
21513515 1S0.0 930721.0 cm-1
21512517 3S1.0 982752.0 cm-1
21512517 1S0.0 989402.0 cm-1
21512518 3P4.0 998931.0 cm-1
21512518 1P1.0 1000920.0 cm-1
21512519 3D7.0 1007400.0 cm-1
2151251a 3F10.0 1011630.0 cm-1
21512519 1D2.0 1012030.0 cm-1
2151251a 1F3.0 1012130.0 cm-1
21513518 1P1.0 1109230.0 cm-1
21513518 3D7.0 1110700.0 cm-1
21513518 3S1.0 1112820.0 cm-1
21513518 3P4.0 1115470.0 cm-1
21513518 1D2.0 1119150.0 cm-1
21513518 1S0.0 1125950.0 cm-1
---------------------------------------------------------------------------------

     Generated from Cowan Atomic Structure Program

     M O'Mullane        14:58   8/07/1994



     SCF method used                      : HR

     Scale factors for Slater Parameters  : 85 99 75 80 65

     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  :  8,all

     Parity 1    Parity 2    Allowed
          545           0        395     initially
          240           0        174     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