ls#n0.dat
Resolved Specific Ion Data Collections
- Ion
- N0+
- Temperature Range
- 0.086 eV → 17.23 eV
ADF04
- Filename
- ls#n0.dat
- Full Path
- adf04/copmm#7/ls#n0.dat
Download data
- Spontaneous Emission: N+0(i) → N+0(j) + hv
- Electron Impact Excitation: N+0(i) + e → N+0(j) + e
| 21522533 4S1.5 | 0.0 cm-1 |
| 21522533 2D4.5 | 19202.5 cm-1 |
| 21522533 2P2.5 | 29144.9 cm-1 |
| 21522523514 4P5.5 | 83406.5 cm-1 |
| 21522523514 2P2.5 | 84770.2 cm-1 |
| 21512543 4P5.5 | 89048.2 cm-1 |
| 21522523515 2S0.5 | 93866.3 cm-1 |
| 21522523515 4D9.5 | 94440.0 cm-1 |
| 21522523515 4P5.5 | 94825.3 cm-1 |
| 21522523515 2D4.5 | 96330.4 cm-1 |
| 21522523515 4S1.5 | 96954.1 cm-1 |
| 21522523515 2P2.5 | 97160.2 cm-1 |
| 21522523514 2D4.5 | 98853.3 cm-1 |
| 21522523516 2P2.5 | 104204.0 cm-1 |
| 21522523516 4F13.5 | 104297.0 cm-1 |
| 21522523516 4P5.5 | 104361.0 cm-1 |
| 21522523516 2F6.5 | 104394.0 cm-1 |
| 21522523516 4D9.5 | 104496.0 cm-1 |
| 21522523516 2D4.5 | 104598.0 cm-1 |
| 21522523515 2F6.5 | 109871.0 cm-1 |
| 21522523515 2D4.5 | 110906.0 cm-1 |
| 21522523515 2P2.5 | 111356.0 cm-1 |
| 21512543 2D4.5 | 117186.0 cm-1 |
| 21522523516 2F6.5 | 119286.0 cm-1 |
| 21522523516 2S0.5 | 119463.0 cm-1 |
| 21522523516 2G8.5 | 119490.0 cm-1 |
| 21522523516 2P2.5 | 119591.0 cm-1 |
| 21522523516 2D4.5 | 120356.0 cm-1 |
| 21522523514 2S0.5 | 121320.0 cm-1 |
| 21522523515 2P2.5 | 132967.0 cm-1 |
| 21512543 2S0.5 | 137459.0 cm-1 |
| 21512543 2P2.5 | 138192.0 cm-1 |
| 21522523516 2D4.5 | 142032.0 cm-1 |
| 21553 2P2.5 | 258678.0 cm-1 |
--------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program M O'Mullane 16:48 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 : both Optically forbidden transitions E2 : both Born Collision-Strength - print : 9 - forbidden : 0 -> 2 - allowed : 1 -> 1 - included : 3,all Parity 1 Parity 2 Allowed 351 813 868 initially 91 188 267 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 -------------------------------------------------------------------------------