ls#f2.dat
Resolved Specific Ion Data Collections
- Ion
- F2+
- Temperature Range
- 0.776 eV → 155 eV
ADF04
- Filename
- ls#f2.dat
- Full Path
- adf04/copmm#9/ls#f2.dat
Download data
- Spontaneous Emission: F+2(i) → F+2(j) + hv
- Electron Impact Excitation: F+2(i) + e → F+2(j) + e
| 21522533 4S1.5 | 0.0 cm-1 |
| 21522533 2D4.5 | 31860.0 cm-1 |
| 21522533 2P2.5 | 49126.0 cm-1 |
| 21512543 4P5.5 | 169193.0 cm-1 |
| 21512543 2D4.5 | 214523.0 cm-1 |
| 21512543 2P2.5 | 242685.0 cm-1 |
| 21512543 2S0.5 | 246075.0 cm-1 |
| 21522523514 4P5.5 | 317875.0 cm-1 |
| 21522523514 2P2.5 | 321843.0 cm-1 |
| 21522523514 2D4.5 | 342273.0 cm-1 |
| 21522523515 2S0.5 | 348376.0 cm-1 |
| 21522523515 4D9.5 | 350552.0 cm-1 |
| 21522523515 4P5.5 | 352012.0 cm-1 |
| 21522523515 2D4.5 | 356298.0 cm-1 |
| 21522523515 4S1.5 | 358858.0 cm-1 |
| 21522523515 2P2.5 | 359187.0 cm-1 |
| 21522523515 2F6.5 | 375387.0 cm-1 |
| 21522523514 2S0.5 | 376881.0 cm-1 |
| 21522523515 2D4.5 | 379432.0 cm-1 |
| 21522523515 2P2.5 | 381409.0 cm-1 |
| 21522523516 4F13.5 | 387982.0 cm-1 |
| 21522523516 2P2.5 | 389014.0 cm-1 |
| 21522523516 4D9.5 | 389534.0 cm-1 |
| 21522523516 4P5.5 | 389885.0 cm-1 |
| 21522523516 2F6.5 | 390759.0 cm-1 |
| 21522523516 2D4.5 | 393220.0 cm-1 |
| 21522523516 2F6.5 | 411845.0 cm-1 |
| 21522523515 2P2.5 | 412095.0 cm-1 |
| 21522523516 2G8.5 | 412727.0 cm-1 |
| 21522523516 2D4.5 | 413451.0 cm-1 |
| 21522523516 2P2.5 | 414744.0 cm-1 |
| 21522523516 2S0.5 | 416659.0 cm-1 |
| 21553 2P2.5 | 419022.0 cm-1 |
| 21522523516 2D4.5 | 447789.0 cm-1 |
--------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program M O'Mullane 14:56 8/07/1994 SCF method used : HR Scale factors for Slater Parameters : 85 95 60 55 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 358 0 868 initially 91 0 267 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 -------------------------------------------------------------------------------