ls#n3.dat
Resolved Specific Ion Data Collections
- Ion
- N3+
- Temperature Range
- 1.379 eV → 276 eV
ADF04
- Filename
- ls#n3.dat
- Full Path
- adf04/copmm#7/ls#n3.dat
Download data
- Spontaneous Emission: N+3(i) → N+3(j) + hv
- Electron Impact Excitation: N+3(i) + e → N+3(j) + e
| 21522 1S0.0 | 0.0 cm-1 |
| 21512513 3P4.0 | 62303.6 cm-1 |
| 21512513 1P1.0 | 122275.0 cm-1 |
| 21523 3P4.0 | 169496.0 cm-1 |
| 21523 1D2.0 | 186200.0 cm-1 |
| 21523 1S0.0 | 222590.0 cm-1 |
| 21512514 3S1.0 | 372091.0 cm-1 |
| 21512514 1S0.0 | 382950.0 cm-1 |
| 21512515 3P4.0 | 401063.0 cm-1 |
| 21512515 1P1.0 | 405347.0 cm-1 |
| 21512516 3D7.0 | 414423.0 cm-1 |
| 21512516 1D2.0 | 422709.0 cm-1 |
| 21513515 1P1.0 | 474895.0 cm-1 |
| 21513515 3D7.0 | 477611.0 cm-1 |
| 21513515 3S1.0 | 480525.0 cm-1 |
| 21513515 3P4.0 | 489125.0 cm-1 |
| 21512517 1S0.0 | 491425.0 cm-1 |
| 21512517 3S1.0 | 491791.0 cm-1 |
| 21513515 1D2.0 | 495134.0 cm-1 |
| 21512518 3P4.0 | 501668.0 cm-1 |
| 21512518 1P1.0 | 503082.0 cm-1 |
| 21512519 3D7.0 | 507033.0 cm-1 |
| 21513515 1S0.0 | 509090.0 cm-1 |
| 2151251a 3F10.0 | 509585.0 cm-1 |
| 2151251a 1F3.0 | 509805.0 cm-1 |
| 21512519 1D2.0 | 510115.0 cm-1 |
| 21513518 1P1.0 | 580331.0 cm-1 |
| 21513518 3D7.0 | 581188.0 cm-1 |
| 21513518 3S1.0 | 582549.0 cm-1 |
| 21513518 3P4.0 | 584756.0 cm-1 |
| 21513518 1D2.0 | 587251.0 cm-1 |
| 21513518 1S0.0 | 592341.0 cm-1 |
--------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program M O'Mullane 16:49 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 544 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 -------------------------------------------------------------------------------