cllike_al97#fe9.dat
Resolved Specific Ion Data Collections
- Ion
- Fe9+
- Temperature Range
- 4.308 eV → 8617 eV
ADF04
- Filename
- cllike_al97#fe9.dat
- Full Path
- adf04/cllike/cllike_al97#fe9.dat
Download data
- Spontaneous Emission: Fe+9(i) → Fe+9(j) + hv
- Electron Impact Excitation: Fe+9(i) + e → Fe+9(j) + e
| 3s2.3p5 2P1.5 | 0.0 cm-1 |
| 3s2.3p5 2P0.5 | 15683.1 cm-1 |
| 3s.3p6 2S0.5 | 289249.0 cm-1 |
| 3s2.3p4(3p).3d 4D2.5 | 388674.0 cm-1 |
| 3s2.3p4(3p).3d 4D3.5 | 388744.0 cm-1 |
| 3s2.3p4(3p).3d 4D1.5 | 390050.0 cm-1 |
| 3s2.3p4(3p).3d 4D0.5 | 391555.0 cm-1 |
| 3s2.3p4(3p).3d 4F4.5 | 417653.0 cm-1 |
| 3s2.3p4(1d).3d 2P0.5 | 426926.0 cm-1 |
| 3s2.3p4(3p).3d 4F3.5 | 422795.0 cm-1 |
| 3s2.3p4(3p).3d 4F2.5 | 426707.0 cm-1 |
| 3s2.3p4(1d).3d 2P1.5 | 428002.0 cm-1 |
| 3s2.3p4(3p).3d 4F1.5 | 428298.0 cm-1 |
| 3s2.3p4(1d).3d 2D1.5 | 434614.0 cm-1 |
| 3s2.3p4(3p).3d 4P0.5 | 434800.0 cm-1 |
| 3s2.3p4(3p).3d 2F3.5 | 440840.0 cm-1 |
| 3s2.3p4(3p).3d 4P2.5 | 441853.0 cm-1 |
| 3s2.3p4(3p).3d 4P1.5 | 442439.0 cm-1 |
| 3s2.3p4(1d).3d 2D2.5 | 444127.0 cm-1 |
| 3s2.3p4(1d).3d 2G4.5 | 450751.0 cm-1 |
| 3s2.3p4(1d).3d 2G3.5 | 451084.0 cm-1 |
| 3s2.3p4(3p).3d 2F2.5 | 452730.0 cm-1 |
| 3s2.3p4(1d).3d 2F2.5 | 482052.0 cm-1 |
| 3s2.3p4(1d).3d 2F3.5 | 485983.0 cm-1 |
| 3s2.3p4(1s).3d 2D1.5 | 511800.0 cm-1 |
| 3s2.3p4(1s).3d 2D2.5 | 516222.0 cm-1 |
| 3s2.3p4(1d).3d 2S0.5 | 541879.0 cm-1 |
| 3s2.3p4(3p).3d 2P1.5 | 564198.0 cm-1 |
| 3s2.3p4(3p).3d 2P0.5 | 569985.0 cm-1 |
| 3s2.3p4(3p).3d 2D2.5 | 572954.0 cm-1 |
| 3s2.3p4(3p).3d 2D1.5 | 586244.0 cm-1 |
| 3s.3p5.3d 4P0.5 | 710847.0 cm-1 |
| 3s.3p5.3d 4P1.5 | 713657.0 cm-1 |
| 3s.3p5.3d 4P2.5 | 718610.0 cm-1 |
| 3s.3p5(3p*).3d 4F4.5 | 696661.0 cm-1 |
| 3s.3p5(3p*).3d 4F3.5 | 699492.0 cm-1 |
| 3s.3p5(3p*).3d 4F2.5 | 702585.0 cm-1 |
| 3s.3p5(3p*).3d 4F1.5 | 705430.0 cm-1 |
| 3s.3p5.3d 4D3.5 | 767016.0 cm-1 |
| 3s.3p5.3d 4D0.5 | 768803.0 cm-1 |
| 3s.3p5.3d 4D2.5 | 768706.0 cm-1 |
| 3s.3p5.3d 4D1.5 | 769040.0 cm-1 |
| 3s.3p5.3d 2F3.5 | 793218.0 cm-1 |
| 3s.3p5.3d 2D2.5 | 801941.0 cm-1 |
| 3s.3p5.3d 2D1.5 | 799385.0 cm-1 |
| 3s.3p5.3d 2F2.5 | 796186.0 cm-1 |
| 3s.3p5.3d 2P0.5 | 827105.0 cm-1 |
| 3s.3p5.3d 2P1.5 | 834924.0 cm-1 |
| 3s.3p5.3d 2F2.5 | 870966.0 cm-1 |
| 3s.3p5.3d 2F3.5 | 872220.0 cm-1 |
| 3s.3p5.3d 2D1.5 | 899365.0 cm-1 |
| 3s.3p5.3d 2D2.5 | 900183.0 cm-1 |
| 3s.3p5.3d 2P0.5 | 975260.0 cm-1 |
| 3s.3p5.3d 2P1.5 | 974116.0 cm-1 |
Contributors
- Alessandro Lanzafame
- CHIANTI
- Keith Berrington
----------------------------------------------------------------------------- Date :Tue Oct 21, 1997 File generated by Alessandro Lanzafame using C2ADAS (conversion from CHIANTI 1.01 database) Ionisation potential from ~adas/adf04/copmm#26/ic#fe9.dat References (from CHIANTI 1.01 data files): Energy levels: energy levels(11,12,18,19,22,26): Jupen et al. MNRAS 264 627 1994 energy levels(1-8,10,13-17,20-21,23-25,27-31,35-38): NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61, 1995. Theoretical energy levels: Bhatia & Doschek, ADNDT, 60, 97, 1995 NOTE: The third energy column contains energy levels derived from "superstructure", and were used to give the theoretical wavelengths in the .wgfa file. To get these energies, the superstructure energies were adjusted by amounts estimated from comparing the theoretical with the observed energies for neighbouring levels. (For the 3s.3p5.3d config the 4F levels were used.) Levels 4 and 5 are observed to have the same energy (388709 cm^-1) but this leads to problems in level population programs so have split the two levels using the difference from the SUPERSTRUCTURE model (i.e. 70 cm^-1).C Oscillator strengths: Tansition probabilities from superstructure includes all allowed t.p.s from levels 1-54 includes all forbidden t.p.s from metastables Collision strengths: Data from Pelan and Berrington AA (1994) for the 1-2 transition. The upsilons are accurate for the range 10^5 - 10^7 K ----------------------------------------------------------------------- --------------------------------------------------------------------------------- ---------------------------------------------------------------------------------