cop98#10_ic#ne4.dat
Resolved Specific Ion Data Collections
- Ion
- Ne4+
- Temperature Range
- 1.077 eV → 1077 eV
ADF04
- Filename
- cop98#10_ic#ne4.dat
- Full Path
- adf04/adas#10/cop98#10_ic#ne4.dat
Download data
- Spontaneous Emission: Ne+4(i) → Ne+4(j) + hv
- Electron Impact Excitation: Ne+4(i) + e → Ne+4(j) + e
| 1s2 2s2 2p2 3P0.0 | 0.0 cm-1 |
| 1s2 2s2 2p2 3P1.0 | 412.0 cm-1 |
| 1s2 2s2 2p2 3P2.0 | 1110.0 cm-1 |
| 1s2 2s2 2p2 1D2.0 | 30291.0 cm-1 |
| 1s2 2s2 2p2 1S0.0 | 63914.0 cm-1 |
| 1s2 2s1 2p3 5S2.0 | 88360.0 cm-1 |
| 1s2 2s1 2p3 3D3.0 | 175834.0 cm-1 |
| 1s2 2s1 2p3 3D2.0 | 175905.0 cm-1 |
| 1s2 2s1 2p3 3D1.0 | 175926.0 cm-1 |
| 1s2 2s1 2p3 3P2.0 | 208157.0 cm-1 |
| 1s2 2s1 2p3 3P1.0 | 208158.0 cm-1 |
| 1s2 2s1 2p3 3P0.0 | 208193.0 cm-1 |
| 1s2 2s1 2p3 1D2.0 | 270564.0 cm-1 |
| 1s2 2s1 2p3 3S1.0 | 279365.0 cm-1 |
| 1s2 2s1 2p3 1P1.0 | 303812.0 cm-1 |
| 1s2 2p4 3P2.0 | 412681.0 cm-1 |
| 1s2 2p4 3P1.0 | 413466.0 cm-1 |
| 1s2 2p4 3P0.0 | 413803.0 cm-1 |
| 1s2 2p4 1D2.0 | 458113.0 cm-1 |
| 1s2 2p4 1S0.0 | 525541.0 cm-1 |
| 2s2 2p1 3s1 3P0.0 | 596254.0 cm-1 |
| 2s2 2p1 3s1 3P1.0 | 596626.0 cm-1 |
| 2s2 2p1 3s1 3P2.0 | 597523.0 cm-1 |
| 2s2 2p1 3s1 1P1.0 | 605231.0 cm-1 |
| 2s2 2p1 3p1 1P1.0 | 635400.0 cm-1 |
| 2s2 2p1 3p1 3D1.0 | 640422.0 cm-1 |
| 2s2 2p1 3p1 3D2.0 | 640868.0 cm-1 |
| 2s2 2p1 3p1 3D3.0 | 641646.0 cm-1 |
| 2s2 2p1 3p1 3S1.0 | 646370.0 cm-1 |
| 2s2 2p1 3p1 3P0.0 | 650699.0 cm-1 |
| 2s2 2p1 3p1 3P1.0 | 651100.0 cm-1 |
| 2s2 2p1 3p1 3P2.0 | 651600.0 cm-1 |
| 2s2 2p1 3p1 1D2.0 | 663500.0 cm-1 |
| 2s2 2p1 3p1 1S0.0 | 678500.0 cm-1 |
| 2s2 2p1 3d1 3F2.0 | 690000.0 cm-1 |
| 2s2 2p1 3d1 1D2.0 | 690691.0 cm-1 |
| 2s2 2p1 3d1 3F3.0 | 690899.0 cm-1 |
| 2s2 2p1 3d1 3F4.0 | 691500.0 cm-1 |
| 2s2 2p1 3d1 3D1.0 | 698231.0 cm-1 |
| 2s2 2p1 3d1 3D2.0 | 698382.0 cm-1 |
| 2s2 2p1 3d1 3D3.0 | 698735.0 cm-1 |
| 2s2 2p1 3d1 3P2.0 | 701765.0 cm-1 |
| 2s2 2p1 3d1 3P1.0 | 702074.0 cm-1 |
| 2s2 2p1 3d1 1P1.0 | 702412.0 cm-1 |
| 2s2 2p1 3d1 3P0.0 | 702459.0 cm-1 |
| 2s2 2p1 3d1 1F3.0 | 709956.0 cm-1 |
| 2s2 2p1 4s1 3P0.0 | 811825.0 cm-1 |
| 2s2 2p1 4s1 3P1.0 | 812130.0 cm-1 |
| 2s2 2p1 4s1 3P2.0 | 813156.0 cm-1 |
| 2s2 2p1 4s1 1P1.0 | 815103.0 cm-1 |
| 2s2 2p1 4p1 1P1.0 | 827960.0 cm-1 |
| 2s2 2p1 4p1 3D1.0 | 828938.0 cm-1 |
| 2s2 2p1 4p1 3D2.0 | 829149.0 cm-1 |
| 2s2 2p1 4p1 3D3.0 | 829918.0 cm-1 |
| 2s2 2p1 4p1 3S1.0 | 831234.0 cm-1 |
| 2s2 2p1 4p1 3P0.0 | 833768.0 cm-1 |
| 2s2 2p1 4p1 3P1.0 | 834156.0 cm-1 |
| 2s2 2p1 4p1 3P2.0 | 834523.0 cm-1 |
| 2s2 2p1 4p1 1D2.0 | 837680.0 cm-1 |
| 2s2 2p1 4p1 1S0.0 | 843030.0 cm-1 |
| 2s2 2p1 4d1 3F2.0 | 846521.0 cm-1 |
| 2s2 2p1 4d1 3F3.0 | 847149.0 cm-1 |
| 2s2 2p1 4d1 1D2.0 | 847424.0 cm-1 |
| 2s2 2p1 4d1 3F4.0 | 847848.0 cm-1 |
| 2s2 2p1 4d1 3D1.0 | 849531.0 cm-1 |
| 2s2 2p1 4d1 3D2.0 | 849684.0 cm-1 |
| 2s2 2p1 4d1 3D3.0 | 850133.0 cm-1 |
| 2s2 2p1 4d1 3P2.0 | 850839.0 cm-1 |
| 2s2 2p1 4d1 3P1.0 | 851069.0 cm-1 |
| 2s2 2p1 4d1 3P0.0 | 851186.0 cm-1 |
| 2s2 2p1 4f1 1F3.0 | 853879.0 cm-1 |
| 2s2 2p1 4f1 3F2.0 | 853922.0 cm-1 |
| 2s2 2p1 4f1 3F3.0 | 853999.0 cm-1 |
| 2s2 2p1 4f1 3F4.0 | 854064.0 cm-1 |
| 2s2 2p1 4d1 1P1.0 | 854980.0 cm-1 |
| 2s2 2p1 4d1 1F3.0 | 855074.0 cm-1 |
| 2s2 2p1 4f1 3G3.0 | 855246.0 cm-1 |
| 2s2 2p1 4f1 3G4.0 | 855338.0 cm-1 |
| 2s2 2p1 4f1 3G5.0 | 855866.0 cm-1 |
| 2s2 2p1 4f1 3D3.0 | 855914.0 cm-1 |
| 2s2 2p1 4f1 3D2.0 | 855998.0 cm-1 |
| 2s2 2p1 4f1 1G4.0 | 856078.0 cm-1 |
| 2s2 2p1 4f1 3D1.0 | 856404.0 cm-1 |
| 2s2 2p1 4f1 1D2.0 | 856502.0 cm-1 |
| 2s1 2p2 3s1 5P1.0 | 697025.0 cm-1 |
| 2s1 2p2 3s1 5P2.0 | 697577.0 cm-1 |
| 2s1 2p2 3s1 5P3.0 | 698031.0 cm-1 |
Predecessors
Dependents
Contributors
- Martin O'Mullane
- Kanti Aggarwal
- Don Griffin
- Alessandra Giunta
------------------------------------------------------------------------------- Combined two specific ion files Target : /work/work_remote/mog/spec/cop98#10/temp Supplementary : /work/work_remote/mog/adas_work/adas215_adf04.pass These are a filtered /home/mog/adas/adf04/cop98#10/cop98#10_ic#ne4.dat and a temperature regridded /home/adas/adas/adf04/clike/clike_dcg00#ne4.dat. There is no real need to store these intermediate steps. Replace SUPPLEMENTARY level into TARGET level 1 1 2 2 3 3 4 4 5 5 6 6 7 7 8 8 9 9 10 10 11 11 12 12 13 13 14 14 15 15 16 16 17 17 18 18 19 19 20 20 21 21 22 22 23 23 24 24 25 25 26 26 27 27 28 28 29 29 30 30 31 31 32 32 33 33 34 34 35 35 36 36 37 37 38 38 39 85 40 86 41 87 42 39 43 40 44 41 45 42 46 43 47 44 48 45 49 46 Code : /home/omullane/merge_adf04/merge_adf04 Date : 12-Dec-2000 Producer : Martin O'Mullane ------------------------------------------------------------------------------- For the following transitions supplement A values have been used, Check supplement values! Tran. Target Supp Factor 35 2 5.96D+08 4.38D+07 136.07 36 2 3.15D+05 1.67D+08 5301.59 15 3 2.02D+04 6.62D+05 327.72 35 3 4.63D+05 5.64D+07 1218.14 46 3 1.24D+07 1.27D+06 97.64 8 4 4.00D-01 4.20D+04 1050000.00 9 4 3.28D-01 2.91D+04 887195.12 10 4 2.31D-01 4.78D+04 2069264.07 14 4 1.15D+04 1.02D+06 886.96 25 6 1.59D+01 2.88D+02 181.13 29 6 1.28D+04 2.27D+05 177.34 31 6 1.93D+01 2.72D+04 14093.26 32 6 2.25D+00 6.65D+04 295555.56 33 6 7.82D-02 6.56D+01 8388.75 32 7 2.69D+08 2.92D+09 108.55 29 8 8.88D+05 1.59D+07 179.05 31 8 2.39D+08 2.62D+09 109.62 32 8 5.04D+07 5.21D+08 103.37 29 9 3.53D+05 5.62D+06 159.21 30 9 3.22D+08 3.53D+09 109.63 31 9 8.22D+07 8.73D+08 106.20 32 9 3.45D+06 3.46D+07 100.29 34 9 1.81D+05 2.11D+06 116.57 31 10 1.80D+06 9.31D+07 517.22 32 10 1.57D+05 3.21D+08 20445.86 33 10 8.49D+02 2.04D+05 2402.83 30 11 6.33D+05 3.84D+08 6066.35 31 11 9.32D+04 1.52D+08 16309.01 32 11 5.36D+03 1.15D+08 214552.24 34 11 4.37D+02 9.97D+05 22814.65 31 12 8.90D+03 1.73D+08 194382.02 25 14 9.73D+02 1.61D+05 1654.68 29 14 7.02D+03 1.50D+05 213.68 30 14 5.65D+04 1.41D+07 2495.58 31 14 4.57D+04 1.46D+07 3194.75 32 14 4.18D+04 1.60D+07 3827.75 33 14 3.14D+04 4.17D+05 132.80 16 15 7.14D-01 1.15D+05 1610644.26 25 15 9.80D+05 1.27D+08 1295.92 26 15 1.76D+04 9.61D+05 546.02 29 15 2.32D+03 1.81D+05 780.17 31 15 7.18D+02 1.91D+04 266.02 22 16 3.50D+06 7.60D+04 460.53 23 16 6.48D+06 1.36D+05 476.47 24 16 5.97D+04 5.40D+01 11055.56 35 16 1.47D+05 3.80D+02 3868.42 37 16 5.27D+05 1.87D+03 2818.18 39 16 2.73D+06 3.06D+04 892.16 40 16 2.65D+07 2.83D+05 936.40 41 16 1.32D+08 1.52D+06 868.42 42 16 1.68D+07 2.61D+05 643.68 43 16 6.60D+06 7.27D+04 907.84 46 16 3.06D+05 3.82D+02 8010.47 21 17 8.34D+06 1.84D+05 453.26 22 17 2.08D+06 4.56D+04 456.14 23 17 2.13D+06 4.55D+04 468.13 24 17 1.64D+04 9.35D+01 1754.01 35 17 4.25D+05 5.07D+02 8382.64 39 17 5.09D+07 6.04D+05 842.72 40 17 1.01D+08 1.26D+06 801.59 43 17 6.99D+06 1.16D+05 602.59 44 17 6.81D+04 2.51D+03 271.31 45 17 1.32D+07 1.92D+05 687.50 22 18 2.78D+06 6.07D+04 457.99 24 18 7.82D+03 4.85D+02 161.24 39 18 7.54D+07 9.58D+05 787.06 43 18 1.21D+06 3.36D+04 360.12 44 18 3.44D+04 2.53D+01 13596.84 22 19 8.79D+04 6.45D+01 13627.91 23 19 1.04D+03 1.79D+01 581.01 24 19 1.23D+07 1.02D+05 1205.88 35 19 4.39D+07 1.41D+04 31134.75 36 19 5.82D+07 1.97D+05 2954.31 37 19 5.26D+04 5.77D+02 911.61 39 19 2.88D+04 1.26D+03 228.57 40 19 2.22D+05 1.07D+03 2074.77 41 19 1.36D+05 2.53D+03 537.55 42 19 1.47D+05 8.17D+01 17992.66 43 19 2.35D+04 4.64D+02 506.47 44 19 2.07D+07 1.43D+06 144.76 46 19 7.69D+07 7.13D+05 1078.54 22 20 2.22D+04 2.14D+01 10373.83 24 20 4.28D+06 3.33D+03 12852.85 39 20 2.06D+05 8.34D+03 247.00 43 20 1.05D+05 2.43D+03 432.10 44 20 1.60D+08 8.39D+06 190.70 25 23 4.22D+02 2.86D+01 147.55 36 27 2.51D+07 2.56D+06 98.05 44 27 2.48D+03 3.40D-01 72941.18 35 29 2.80D+03 4.09D+00 6845.97 35 31 1.84D+05 2.38D+03 773.11 36 31 4.62D+00 2.38D+04 51515.15 37 32 1.84D+05 1.54D+04 119.48 46 32 1.51D+05 7.21D+03 209.43 41 33 1.16D+04 1.27D+03 91.34 43 33 9.46D+03 5.24D+00 18053.44 ------------------------------------------------------------------------------- Comments from target file ------------------------------------------------------------------------------- Combined two specific ion files Target : /home/omullane/adas/adf04/cop98#10/copmm#10_ic#ne4.dat Supplementary : /home/omullane/adas/adf04/clike/test.dat Replace SUPPLEMENTARY level into TARGET level 1 1 2 2 3 3 4 4 5 5 6 6 7 8 8 7 9 9 10 10 11 11 12 12 13 13 14 14 15 15 16 18 17 17 18 16 19 19 20 20 Code : /home/omullane/merge_adf04/merge_adf04 Date : 18-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 3 1 7.04D-09 1.00D-30 5 1 0.00D+00 1.00D-30 18 1 0.00D+00 1.00D-30 20 1 0.00D+00 1.00D-30 18 5 0.00D+00 1.00D-30 20 5 0.00D+00 1.00D-30 18 16 2.83D-08 1.00D-30 20 18 0.00D+00 1.00D-30 10 6 5.03D-07 2.01D-07 13 10 1.08D+00 5.47D-07 15 14 6.04D-01 1.00D-30 Choice of A values for the following transitions has been made 3 1, 5 1, 18 1, 20 1, 18 5, 20 5, 18 16, 20 18 10 6, 13 10, 15 14 ------------------------------------------------------------------------------- For the following transitions supplement A values have been used Check supplement values Tran. Target Supp 3 1 7.04D-09 1.00D-30 17 2 1.53D+03 2.51D+00 16 5 2.04D-04 3.63D-02 18 16 2.83D-08 1.00D-30 10 7 1.74D+04 1.70D+00 11 9 9.05D+00 7.94D-01 13 9 1.68D-02 2.39D-01 14 9 1.52D+01 1.57D-02 15 9 5.35D-01 4.64D-05 13 10 1.08D+00 5.47D-07 14 13 5.53D-09 1.65D-06 15 14 6.04D-01 1.00D-30 15 3 3.23D+05 2.02D+04 7 4 5.75D+04 4.00D-01 8 4 3.09D+04 3.28D-01 12 4 2.80D+04 2.31D-01 14 4 2.72D+05 1.15D+04 16 15 8.64D+04 7.14D-01 ------------------------------------------------------------------------------- Comments from target file --------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program From IFG file : ne4#IFG M G O'Mullane 18-Nov-9 SCF method used : HR Scale factors for Slater Parameters : 98 99 90 90 65 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 634 713 1097 initially 634 713 1097 reduced --------------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------------- File generated by expansion of an LS-resolved file Program: ADAS210 Source file : /u/mog/adas/adf04/clike_kma84#ne4b.dat Template file : /u/adas/adas/adf04/copmm#10/copmm#10_ne4j.dat Output file : /u/mog/adas/adf04/work/clike_kma84#ne4b_exp.dat Template File 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 Source File Assignment: 1 1 1 2 3 4 5 5 5 6 6 6 7 8 9 10 10 10 11 12 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 Altered the temperature set with ADAS215 Source file: /home/mog/adas/adf04/work/clike_kma84#ne4b_exp.dat Producer: Martin O'Mullane Date: 02/10/98 ------------------------------------------------------------------------------- File generated by altering the temperature set of an ADF04 file Program: ADAS215 Source file: /home/mog/adas/adf04/work/clike_kma84#ne4a.dat Producer: Martin O'Mullane Date: 04/10/98 ------------------------------------------------------------------------------- File generated by altering the temperature set of an ADF04 file Program: ADAS215 Source file: /home/mog/adas/adf04/work/clike_kma84#ne4c.dat Producer: Martin O'Mullane Date: 04/10/98 ------------------------------------------------------------------------------- Assembled from 3 papers of Aggarwal. Unfortunately these were over three temperature ranges and two resolutions so a degree of extrapolation with ADAS215 was required. The allowed electric dipole transitions were only given in LS resolution; these were unbundled with ADAS210. See above comments for details. K M Aggarwal, Astro. J. Suppl. 54, p1-15, 1984 K M Aggarwal, Astro. J. Suppl. 58, p289-296, 1985 K M Aggarwal, Astro. J. Suppl. 61, p699-717, 1986 The A-values are those of Aggarwal supplemented by those of A K Bathia and G A Doschek, ADNDT, 55, p315-348, 1993. Note that there is some disagreement in the A values between these papers, sometimes up to a factor of 2. It was decided to adopt the A value from the same calculation of the collision strength where this was available. Also note that there is some dispute in the literature regarding the accuracy of the Aggarwal allowed collision strengths (cf Burgess, Mason and Tully, Astro. J. 376, p803-808, 1991) Martin O'Mullane 4/10/98 ------------------------------------------------------------------------------- Energy levels from NIST data up to n=3. Levels 19 and 20 from 1s2 2p4 were not available. Comparison of the Cowan values and other theoretical calculations reported in Aggarwal AJ Sup. Ser. 118:589-602, 1998 do not give a compelling reason for replacing the Cowan values with the others. There is very littles NIST data for the n=4 levels and what is there is term averaged and not from observation. Therefore the Cowan values are preferred. Martin O'Mullane 18/10/98 ------------------------------------------------------------------------------- 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 73 74 75 76 77 78 79 80 81 82 83 84 Original level order : 1 2 3 4 5 6 9 7 8 12 11 10 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 36 35 37 38 39 40 41 42 43 46 44 45 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 73 74 75 76 77 78 79 80 81 82 83 84 Unphysical A values. Set A=1.0E-30 for following transitions : 36 35 A = 2.74D-03 46 44 A = 6.30D-12 Date : 12-Dec-00 Producer : Martin O'Mullane -------------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------------- File generated by altering the temperature set of an ADF04 file Program : ADAS215 Source file : /home/adas/adas/adf04/clike/clike_dcg00#ne4.dat Producer : Martin O'Mullane Date : 12/12/00 Original comments June 5, 2000 From a 66-term 138-level Intermediate-Coupling Frame Transformation (ICFT) R-matrix calculation that included all levels of the configurations 2s22p2, 2p4, 2s2p3, 2s22p3s, 2s22p3p, 2s22p3d, and 2s2p23s, 2s22p4s, 2s23p4p, 2s22p4d; and all the levels in 2s2p23p and 2s2p23d that lie below the highest level of 2s22p4d. In addition the remaining levels of 2s2p23p and 2s2p23d and all the levels of 2p33s, 2p33p, and 2p33d were included in the CI expansion. The 1s, 2s, and 2p orbitals were determined from a single-configuration Hartree-Fock calculation on 2s22p2 3P. The 3s, 3p, and 3d orbitals were determined from multi-configuration Hartree-Fock calculations on 2s22p3s+2P33s 3P, 2s22p3p+2p33p 3D, and 2s22p3d+2p33d 3F, respectively, and the 4s, 4p, and 4d orbitals were determined from single-configuration Hartree-Fock calculations on 1s22p4l. In STG3 of the R-matrix calculation, the term energies were adjusted to the experimental term energies and in the ICFT calculation, the level energies were adjusted to the experimental values where known. For the JPI partial waves from J=0.5 to 9.5 and even and odd parity, we performed an LS R-matrix calculation with exchange for the LSPI partial waves with L = 0 to L = 12 and then transformed the unphysical K-matrices to intermediate coupling using the ICFT method. For the higher partial waves, we performed a no-exchange calculation in LS coupling, with the long-range multipoles included, for all LSPI partial waves from L = 8 to 40; transformed the unphysical K-matrices to intermediate-coupling; and topped up. This allowed us to add the partial-wave contributions from J = 10.5 to 37.5. The size of the continuum basis for these calculations was set to 24. The radiative rates for the dipole-allowed transitions were determined from our 138-level CI calculation in the Breit-Pauli approximation. The number of mesh points used in the asymptotic part of the problem was 8740 and the maximum energy was 15 Ry. Donald C. Griffin Published in J. Phys. B, 33, p4389-4408, (2000). -------------------------------------------------------------------------------C------------------------------------------------------------------------------- Added transition probabilities for intercombination lines, 6-2, 6-3 and 6-4 from C Mendoza et al, Astron. Astro. Supp., 135, p159-169, (1999). Author : Martin O'Mullane Date : 12-12-2000 ------------------------------------------------------------------------------- Configurations 85, 86 and 87 incorrectely identified as 2S2 2P2 3S1 - they should be 2S1 2P2 3S1. Producer : Alessandra Giunta Date : 29-06-2012 ------------------------------------------------------------------------------- --------------------------------------------------------------------------------- ---------------------------------------------------------------------------------