cop98#10_ls#ne3.dat
Resolved Specific Ion Data Collections
- Ion
- Ne3+
- Temperature Range
- 0.689 eV → 1379 eV
ADF04
- Filename
- cop98#10_ls#ne3.dat
- Full Path
- adf04/adas#10/cop98#10_ls#ne3.dat
Download data
- Spontaneous Emission: Ne+3(i) → Ne+3(j) + hv
- Electron Impact Excitation: Ne+3(i) + e → Ne+3(j) + e
- Free Electron Recombination: Ne+4(i) + e → Ne+3(j)
| 2s2 2p3 4S1.5 | 0.0 cm-1 |
| 2s2 2p3 2D4.5 | 41252.6 cm-1 |
| 2s2 2p3 2P2.5 | 62439.1 cm-1 |
| 2s1 2p4 4P5.5 | 184222.0 cm-1 |
| 2s1 2p4 2D4.5 | 254089.0 cm-1 |
| 2s1 2p4 2S0.5 | 299628.0 cm-1 |
| 2s1 2p4 2P2.5 | 320267.0 cm-1 |
| 2s2 2p2 3s1 4P5.5 | 479309.0 cm-1 |
| 2p5 2P2.5 | 485225.0 cm-1 |
| 2s2 2p2 3s1 2P2.5 | 488969.0 cm-1 |
| 2s2 2p2 3s1 2D4.5 | 511696.0 cm-1 |
| 2s2 2p2 3p1 2S0.5 | 518571.0 cm-1 |
| 2s2 2p2 3p1 4D9.5 | 521643.0 cm-1 |
| 2s2 2p2 3p1 4P5.5 | 524818.0 cm-1 |
| 2s2 2p2 3p1 2D4.5 | 531208.0 cm-1 |
| 2s2 2p2 3p1 4S1.5 | 532978.0 cm-1 |
| 2s2 2p2 3p1 2P2.5 | 538472.0 cm-1 |
| 2s2 2p2 3s1 2S0.5 | 551989.0 cm-1 |
| 2s2 2p2 3p1 2F6.5 | 555368.0 cm-1 |
| 2s2 2p2 3p1 2D4.5 | 561168.0 cm-1 |
| 2s2 2p2 3p1 2P2.5 | 569412.0 cm-1 |
| 2s2 2p2 3d1 4F13.5 | 574363.0 cm-1 |
| 2s2 2p2 3d1 2P2.5 | 576378.0 cm-1 |
| 2s2 2p2 3d1 4D9.5 | 577942.0 cm-1 |
| 2s2 2p2 3d1 4P5.5 | 579485.0 cm-1 |
| 2s2 2p2 3d1 2F6.5 | 580087.0 cm-1 |
| 2s2 2p2 3d1 2D4.5 | 587111.0 cm-1 |
| 2s2 2p2 3p1 2P2.5 | 602796.0 cm-1 |
| 2s2 2p2 3d1 2F6.5 | 605770.0 cm-1 |
| 2s2 2p2 3d1 2G8.5 | 607046.0 cm-1 |
| 2s2 2p2 3d1 2D4.5 | 609432.0 cm-1 |
| 2s2 2p2 3d1 2P2.5 | 613024.0 cm-1 |
| 2s2 2p2 3d1 2S0.5 | 616759.0 cm-1 |
| 2s2 2p2 3d1 2D4.5 | 651374.0 cm-1 |
Predecessors
Dependents
Contributors
- Martin O'Mullane
- CHIANTI
- Nigel Badnell
------------------------------------------------------------------------------- File generated by compression of a J-resolved file Program: ADAS209 Source file: /home/mog/adas/adf04/cop98#10/cop98#10_ic#ne3.dat Original level indexing: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 Selection Vector: 1 2 2 3 3 4 4 4 5 5 6 7 7 8 8 8 9 9 10 10 11 12 11 13 13 13 13 14 14 14 15 15 16 17 17 18 19 19 20 20 21 21 22 22 22 22 23 23 24 24 24 24 25 25 26 25 26 27 27 28 28 29 29 30 30 31 31 32 32 33 34 34 Original parent metastables: (1S) Parent bundling vector: 0 Insert producer id here: Date: 08/03/00 ------------------------------------------------------------------------------- Comments from uncompressed file ------------------------------------------------------------------------------- Combined two specific ion files Target : /home/omullane/adas/adf04/cop98#10/copmm#10_ic#ne3.dat Supplementary : /home/omullane/adas/adf04/nlike/nlike_rb98#ne3.dat Replace SUPPLEMENTARY level into TARGET level 1 1 2 2 3 3 4 4 5 5 6 8 7 7 8 6 9 9 10 10 11 11 12 13 13 12 14 14 15 15 16 16 17 20 18 19 19 17 20 18 21 22 22 21 Code : /home/omullane/merge_adf04/merge_adf04 Date : 21-Nov-98 Producer : Martin O Mullane (JET) ------------------------------------------------------------------------------- A value differences were detected for the following transitions and the target values are used. Tran. Target Supp 14 8 6.16D-08 6.58D-08 11 9 3.82D+00 1.00D-30 12 9 3.61D-01 1.00D-30 13 9 2.42D-01 1.00D-30 14 9 6.61D-02 1.00D-30 15 9 5.84D-02 1.00D-30 17 9 8.07D-02 1.00D-30 18 9 1.02D+00 1.00D-30 21 9 4.23D+02 1.00D-30 22 9 1.48D+03 1.00D-30 17 13 1.23D-07 1.24D-07 19 9 1.17D+09 1.00D-30 Choice of A values for the following transitions has been made 14 8, 11 9, 12 9, 13 9, 14 9, 15 9, 17 9, 18 9 21 9, 22 9, 17 13, 16 14, 19 9 ------------------------------------------------------------------------------- For the following transitions supplement A values have been used, Check supplement values! Tran. Target Supp 19 1 2.80D-01 1.12D+01 20 1 1.87D-01 4.13D+01 20 3 1.26D+04 5.95D+02 20 4 2.52D-10 2.43D-02 17 1 1.37D+06 1.34D+05 16 5 2.40D+04 3.09D+01 19 9 1.17D+09 1.00D-30 20 9 1.12D+10 1.17D+09 ------------------------------------------------------------------------------- Comments from target file --------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : ne3#IFG M G O'Mullane 21-Nov-9 SCF method used : HR Scale factors for Slater Parameters : 90 99 90 90 75 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 : 5,all Parity 1 Parity 2 Allowed 2543 2783 3944 initially 2543 2783 3944 reduced --------------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------------- File generated by altering the temperature set of an ADF04 file Program: ADAS215 Source file: /home/omullane/adas/adf04/nlike/nlike_rb98#ne3.dat Producer: Martin O'Mullane Date: 21/11/98 ------------------------------------------------------------------------------- Energy levels: NIST data tables with the disclaimer NB: Unpublished data of R.L. Kelly. NOT evaluated by NIST. A-values: From 2s2 2p3 (levels 1-5) to levels up to 22 use data from the compilation of Bhatia and Kastner (AJ 332 p1063 1988). These A values are different to the Bhatia values in Chianti but there appears to be a reversal problem with the Chianti dataset. All other A values from a Cowan atomic structure run. Upsilons: From C A Ramsbottom and K L Bell, AD&NDT vol.68 No.2 p203-218 (1998) (Article: DT970765) Transition 1-11 has 0.0 but is given a collision strength of 1.47E-4 at 7.0Ryd by Bhatia and Kastner (AJ 332 p1063 1988). Martin O'Mullane 25-09-98 -------------------------------------------------------------------------------- These are the NIST A values from Wiese?? Should we use these? 5.57-03 1 2 C M1 5.90-04 1 3 D E2 5.30-01 1 4 C M1 1.33+00 1 5 C M1 2.50+09 1 6 E E1 2.50+09 1 7 E E1 2.50+09 1 8 E E1 4.80+09 1 14 E E1 4.80+09 1 15 E E1 4.80+09 1 16 E E1 4.60+09 2 9 E E1 3.89-01 2 4 C M1 4.37-01 2 5 C M1 3.30+08 2 10 E E1 6.70+09 2 21 E' E1 4.90+08 2 22 E' E1 1.50+10 2 12 E E1 1.50+09 2 13 E E1 4.90+08 3 9 E E1 1.10-01 3 4 C E2 4.01-01 3 5 C E2 4.90+09 3 10 E E1 1.40+10 3 13 E E1 7.40+08 3 21 E' E1 6.90+09 3 22 E' E1 5.10+09 4 12 E E1 1.20+09 4 13 E E1 6.40+08 4 9 E E1 2.40+09 5 12 E E1 6.20+09 5 13 E E1 1.30+08 5 9 E E1 7.60+08 5 10 E E1 ------------------------------------------------------------------------------------ Replaced energies with NIST data where available. The following levels are from Cowan code : 33,34,41-46,48-51,60,61,64,65,76,78,79,86,87, 89,90,93-102,108-119,121,123-135,142-159 Split in the 62/63 66/67 91/92 from Cowan with the term average from NIST. Martin O'Mullane 21-11-98 -------------------------------------------------------------------------------- Removed the n=4 terms as this causes trouble with ADAS209 and other codes because of the number of transitions (GT 9000). Martin O'Mullane 08-03-2000 -------------------------------------------------------------------------------- Filtered adf04 file to - sort energy levels - remove non physical A values from energy level reversals - remove energies above ionisation potential - remove duplicate transitions Code : /home/omullane/adf04_utils/filter_adf04.x Level list : 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 Original level order : 1 3 2 4 5 6 7 8 10 9 11 12 13 14 15 16 19 20 17 18 22 23 21 24 25 26 27 28 29 30 31 32 35 33 34 38 36 37 39 40 41 42 43 44 45 46 47 52 48 49 50 51 53 54 56 55 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 Unphysical A values. Set A=1.0E-30 for following transitions : 3 2 A = 1.52D-06 19 17 A = 1.12D+04 19 18 A = 5.55D+04 20 17 A = 4.60D+04 20 18 A = 2.32D+04 34 33 A = 5.93D-09 35 33 A = 5.16D-08 49 48 A = 5.17D-04 50 48 A = 2.00D-02 51 48 A = 5.70D-04 56 55 A = 2.60D-10 Date : 08/03/00 Producer : Martin O'Mullane -------------------------------------------------------------------------------C Filter compressed file for ADAS209 introduced duplications. Filtered adf04 file to - sort energy levels - remove non physical A values from energy level reversals - remove energies above ionisation potential - remove duplicate transitions Code : /home/omullane/adf04_utils/filter_adf04.x The following duplicate transitions were found 25 26 Date : 08/03/00 Producer : Martin O'Mullane -------------------------------------------------------------------------------- Ionisation pathways added. The 2s2 2p3 and 2s 2p4 terms have equivalent electrons and the ionisation pathways are distributed between the 2 parents. Code : ADAS807 Producer : Martin O'Mullane Date : 19/12/00 -------------------------------------------------------------------------------- RADIATIVE RECOMBINATION DATA ADDED PROCESSED BY ADAS211 ON : /home/adas/adas/adf08/rrc98#c/rrc98#c_ne4ls.dat Producer : Martin O'Mullane Date : 19/12/00 -------------------------------------------------------------------------------- Dielectronic data is post-processed from Badnell files as follows: /home/adas/adas/adf09/mom93#c/mom93#c_ne4ls22.dat /home/adas/adas/adf09/mom93#c/mom93#c_ne4ls23.dat The cross-referencing file is as follows: /home/adas/adas/adf18/a09_a04/drm96#n/drm96#n_ls#ne3.dat The parent metastable indices are as follows: 1. 2S2 2P2 (3)1( 4.0) 2. 2S2 2P2 (1)2( 2.0) 3. 2S2 2P2 (1)0( 0.0) 4. 2S1 2P3 (5)0( 2.0) Dielectronic data added to 52 existing rad. recom. level sets Producer : Martin O'Mullane Date : 19/12/00 -------------------------------------------------------------------------------- Added ionisation rates (S-lines) from : /home/adas/adas/adf07/szd96#ne/szd96#ne_ne.dat S 1 +1 ISEL = 26 Energy = 783300.00 S 1 +4 ISEL = 27 Energy = 870906.00 S 2 +1 ISEL = 29 Energy = 742047.40 S 2 +2 ISEL = 30 Energy = 771584.40 S 3 +2 ISEL = 33 Energy = 750397.90 S 3 +3 ISEL = 34 Energy = 784020.90 Code : ADAS807 Producer : Martin O'Mullane Date : 19/12/00 -------------------------------------------------------------------------------- Add the orbital energies. Martin O'Mullane 12-12-2019 -------------------------------------------------------------------------------