cop98#10_ls#ne5.dat
Resolved Specific Ion Data Collections
- Ion
- Ne5+
- Temperature Range
- 1.551 eV → 3102 eV
ADF04
- Filename
- cop98#10_ls#ne5.dat
- Full Path
- adf04/adas#10/cop98#10_ls#ne5.dat
Download data
- Spontaneous Emission: Ne+5(i) → Ne+5(j) + hv
- Electron Impact Excitation: Ne+5(i) + e → Ne+5(j) + e
- Free Electron Recombination: Ne+6(i) + e → Ne+5(j)
| 2s2 2p1 2P2.5 | 0.0 cm-1 |
| 2s1 2p2 4P5.5 | 100120.0 cm-1 |
| 2s1 2p2 2D4.5 | 178132.0 cm-1 |
| 2s1 2p2 2S0.5 | 229983.0 cm-1 |
| 2s1 2p2 2P2.5 | 248961.0 cm-1 |
| 2p3 4S1.5 | 320745.0 cm-1 |
| 2p3 2D4.5 | 358699.0 cm-1 |
| 2p3 2P2.5 | 405166.0 cm-1 |
| 2s2 3s1 2S0.5 | 721738.0 cm-1 |
| 2s2 3p1 2P2.5 | 770577.0 cm-1 |
| 2s2 3d1 2D4.5 | 815533.0 cm-1 |
| 2s1 2p1 3s1 4P5.5 | 833478.0 cm-1 |
| 2s1 2p1 3s1 2P2.5 | 855415.0 cm-1 |
| 2s1 2p1 3p1 4D9.5 | 874548.0 cm-1 |
| 2s1 2p1 3p1 2P2.5 | 875631.0 cm-1 |
| 2s1 2p1 3p1 4S1.5 | 875781.0 cm-1 |
| 2s1 2p1 3p1 4P5.5 | 881651.0 cm-1 |
| 2s1 2p1 3p1 2D4.5 | 899708.0 cm-1 |
| 2s1 2p1 3d1 4F13.5 | 907724.0 cm-1 |
| 2s1 2p1 3p1 2S0.5 | 913988.0 cm-1 |
| 2s1 2p1 3d1 4D9.5 | 925678.0 cm-1 |
| 2s1 2p1 3d1 2D4.5 | 927268.0 cm-1 |
| 2s1 2p1 3d1 4P5.5 | 930920.0 cm-1 |
| 2s1 2p1 3s1 2P2.5 | 939388.0 cm-1 |
| 2s1 2p1 3d1 2F6.5 | 945485.0 cm-1 |
| 2s1 2p1 3d1 2P2.5 | 951465.0 cm-1 |
| 2s1 2p1 3p1 2D4.5 | 985212.0 cm-1 |
| 2s1 2p1 3p1 2P2.5 | 986978.0 cm-1 |
| 2s1 2p1 3p1 2S0.5 | 993128.0 cm-1 |
| 2s1 2p1 3d1 2F6.5 | 1021130.0 cm-1 |
| 2p2 3s1 4P5.5 | 1022360.0 cm-1 |
| 2s1 2p1 3d1 2D4.5 | 1029310.0 cm-1 |
| 2s1 2p1 3d1 2P2.5 | 1031460.0 cm-1 |
| 2p2 3s1 2P2.5 | 1037150.0 cm-1 |
| 2p2 3p1 2S0.5 | 1043120.0 cm-1 |
| 2p2 3s1 2D4.5 | 1055360.0 cm-1 |
| 2p2 3p1 4D9.5 | 1061180.0 cm-1 |
| 2p2 3p1 4P5.5 | 1064920.0 cm-1 |
| 2p2 3p1 2D4.5 | 1064940.0 cm-1 |
| 2p2 3p1 2P2.5 | 1072990.0 cm-1 |
| 2p2 3p1 4S1.5 | 1082170.0 cm-1 |
| 2p2 3d1 4F13.5 | 1088490.0 cm-1 |
| 2p2 3p1 2F6.5 | 1095150.0 cm-1 |
| 2p2 3d1 4D9.5 | 1096420.0 cm-1 |
| 2p2 3d1 2P2.5 | 1096640.0 cm-1 |
| 2p2 3d1 2F6.5 | 1103110.0 cm-1 |
| 2p2 3d1 4P5.5 | 1104380.0 cm-1 |
| 2p2 3p1 2D4.5 | 1107490.0 cm-1 |
| 2p2 3p1 2P2.5 | 1118850.0 cm-1 |
| 2p2 3d1 2D4.5 | 1125280.0 cm-1 |
| 2p2 3s1 2S0.5 | 1128740.0 cm-1 |
| 2p2 3d1 2G8.5 | 1132450.0 cm-1 |
| 2p2 3d1 2F6.5 | 1138740.0 cm-1 |
| 2p2 3d1 2D4.5 | 1140690.0 cm-1 |
| 2p2 3d1 2P2.5 | 1141530.0 cm-1 |
| 2p2 3d1 2S0.5 | 1162760.0 cm-1 |
| 2p2 3p1 2P2.5 | 1179510.0 cm-1 |
| 2p2 3d1 2D4.5 | 1217470.0 cm-1 |
Predecessors
Dependents
Contributors
- Martin O'Mullane
- Hugh Summers
- Douglas Sampson
- Hong Zhang
- Peter McWhirter
- Jim Lang
- Alessandro Lanzafame
------------------------------------------------------------------------------- File generated by compression of a J-resolved file Program: ADAS209 Source file: /home/adas/adas/adf04/adas#10/cop98#10_ic#ne5.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 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 Selection Vector: 1 1 2 2 2 3 3 4 5 5 6 7 7 8 8 9 10 10 11 11 13 13 13 14 14 15 15 16 17 16 15 15 18 18 18 19 19 20 20 20 20 21 22 22 22 22 23 23 24 24 24 25 25 26 26 27 27 28 28 29 29 30 31 31 32 32 32 33 33 34 34 35 35 36 37 37 38 38 38 38 39 40 39 39 40 41 41 42 43 43 43 43 44 44 45 45 46 45 46 45 47 47 48 48 48 49 49 50 50 51 51 52 53 53 54 54 55 55 56 56 57 58 58 59 59 Original parent metastables: (1S) Parent bundling vector: 0 Producer : Martin O'Mullane Date : 11/12/2000 ------------------------------------------------------------------------------- Comments from unbundled file ------------------------------------------------------------------------------- Combined two specific ion files Target : /disk3/summers/adas/adf04/cop98#10/copsm#b_sm#ne5j.dat Supplementary : /home/omullane/adas/adf04/blike/blike_jl96#ne5j.dat 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 Code : /home/omullane/merge_adf04/merge_adf04 Date : 21-Nov-98 Producer : Martin O'Mullane ------------------------------------------------------------------------------- For the following transitions supplement A values have been used, Check supplement values! Tran. Target Supp 2 1 0.00D+00 1.95D-02 11 7 1.38D+02 2.61D+03 11 8 8.97D+00 3.42D+02 ------------------------------------------------------------------------------- Comments from target file ------------------------------------------------------------------------------- Description of the Sampson source data set:- This data set gives relativistic distorted wave collision strengths and oscillator strengths for the 22 B-like ions with 6 <= Z <= 27 obtained by Zhang and Sampson (to appearin Vol. ?? of Atomic Data Nuclear Data Tables, ) Source file :- /JETSHP.RBDATA.TEXT The values of the ionization potential were taken from: Boron-like ionisation potential from Kelly Program :- JETSHP.STRIPSAM.FORT(STRIPSAM) Author :- R.W.P.McWhirter Data set produced :- 23/04/96 ------------------------------------------------------------------------------- The Sampson source data has been extended with impact parameter data for transitions between higher levels. Source data set :- /JETSHP.COPSS#B.DATA(SS#NE5J) ------------------------------------------------------------------------------- Update: 17/11/98 HP Summers Adjusted energy levels from NIST (DAS) data Adjustment was not possible for the following: 26, 29, 32, 33, 34, 35, 38, 39, 40, 41, 72, 73, 74, 84-87, 89-92, 95-125 (excl. 106, 107, 117-120). -------------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------------- ENERGY LEVELS AND IONISATION POTENTIAL The ionisation potential is from Kelly (J Phys Chem Ref Data 16, Suppl 1, 1987). The energies are from Edlen (Phys Scripta 28, 483, 1983). The ordering of the levels is as given in the work used for the effective collision strengths. There are differences in energy of up to 152 cm-1 with the data from the NIST discs. TRANSITION PROBABILITIES For the transition between the 1/2 and 3/2 levels of the ground term the multiconfiguration Hartree-Fock Breit-Pauli result of C Froese Fischer (J Phys B 16, 157 1983) is used (1.95-02 s-1). The multiconfiguration Dirac-Fock calculations of Cheng, Kim and Desclaux (ADNDT 24, 111, 1979) yielded 2.83-02 s-1. The results of Dankwort and Trefftz (Astron Astrophys 65, 93, 1978) have been adopted for the majority of transitions. Their calculation used the multiconfiguration Hartree-Fock ansatz with Breit-Pauli corrections. For transitions 3-12, 3-14, 3-15, 4-12, 4-13, 4-14, 4-15, 5-12, 5-13, 5-15, 6-11, 7-11, 8-11, 8-12, 9-11 and 10-11 Dankwort and Trefftz did not give results. Accordingly the results of Merkelis, Vilkas, Gaigalas and Kisielius were used (Phys Scripta 51, 233, 1995). Their calculation employed the stationary second order many-body perturbation theory, the relativistic corrections being included using the Breit-Pauli approximation. EFFECTIVE COLLISION STRENGTHS In their assessment of effective collision strengths for the B-like sequence Sampson, Zhang and Fontes (ADNDT 57, 98, 1994) review the available results. The results of Hayes (J Phys b25, 2649, 1992 were recommended. These were close coupling calculations by the R-matrix method for transitions between the 2s2 2p 2P and 2s 2p2 4P energy terms and from them to the energy terms of the 2s 2p2, 2p3, 2s2 3s, 2s2 3p and 2s2p3s configurations. Sampson et al anticipated the R-matrix close coupling calculations of Zhang, Graziana and Pradhan (Astron Astrophys 283, 319,1994) for the 105 fine structure transitions among the 15 levels of the 2s2 2p, 2s 2p2 and 2p3 configurations. These results are adopted here. The data were obtained electronically and processed into ADF04 format. J Lang A Lanzafame May 1996 Update: 03/08/97 Ralph Dux - Corrected error in indexing in Upsilon rows. Swapped indices 6 and 7 Update: 21/11/98 Martin O'Mullane - Corrected problem with 12 and 13. ----------------------------------------------------------------------------- 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 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 Original level order : 1 2 3 4 5 7 6 8 9 10 11 13 12 14 15 16 17 18 19 20 21 22 23 24 25 26 29 28 32 27 30 31 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 59 60 58 61 62 66 67 65 63 64 68 69 70 71 73 74 72 79 80 75 78 76 77 81 84 82 83 85 86 87 88 89 90 91 92 93 94 96 95 99 97 100 98 101 102 103 104 105 106 107 108 109 111 112 110 113 114 118 117 115 116 119 120 121 122 123 124 125 Unphysical A values. Set A=1.0E-30 for following transitions : 65 63 A = 2.01D+01 67 64 A = 3.88D+00 65 64 A = 1.64D+00 74 72 A = 2.10D-02 74 73 A = 3.65D+02 77 75 A = 5.14D+00 79 75 A = 1.12D+00 79 76 A = 2.27D+00 80 76 A = 3.07D-01 Date : 08/03/00 Producer : Martin O'Mullane -------------------------------------------------------------------------------- Update to the transition probabilities A values of Galavis et al (Astron. & Astrop. Supp. Series, 131, p499 (1998)) This is Iron Project work with superstructure. Authors quote 'complete radiative data set. Comparisons with other calculations and experiments... allow us to conclude that the present work is statistically the most reliable to date'. For trnsitions between the 0.5-1.5 levels of the ground term the new value is 2.012E-02 close to the previous adopted value of 1.95E-02. For spin allowed E1 transitions accuracy is given as 10% in good agreement with Dankwort and Trefftz. For spin forbidded E1 accuracy is 20% apart from 2p3 4S(1.5) - 2s2p2 2L(J) which has unassigned accurracy. Date : 28/09/2000 Producer : Jim Lang/Martin O'Mullane ------------------------------------------------------------------------------- RADIATIVE RECOMBINATION DATA ADDED PROCESSED BY ADAS211 ON : /home/adas/adas/adf08/rrc98#be/rrc98#be_ne6ls.dat Date : 19/12/2000 Producer : Martin O'Mullane ------------------------------------------------------------------------------- Dielectronic data is post-processed from Badnell files as follows: /home/adas/adas/adf09/mom93#be/mom93#be_ne6ls22.dat /home/adas/adas/adf09/mom93#be/mom93#be_ne6ls23.dat The cross-referencing file is as follows: /home/adas/adas/adf18/a09_a04/drm96#b/drm96#b_ls#ne5.dat The parent metastable indices are as follows: 1. 2S2 (1)0( 0.0) 2. 2S1 2P1 (3)1( 4.0) Dielectronic data added to 30 existing rad. recom. level sets Date : 19/12/2000 Producer : Martin O'Mullane ------------------------------------------------------------------------------- Added ionisation rates (S-lines) from : /home/adas/adas/adf07/szd96#ne/szd96#ne_ne.dat S 1 +1 ISEL = 45 Energy = 1272930.00 S 1 +2 ISEL = 46 Energy = 1385138.70 S 2 +2 ISEL = 48 Energy = 1285018.70 Code : ADAS807 Producer : Martin O'Mullane Date : 19/12/00 ------------------------------------------------------------------------------- Ionisation pathways added. The 2s 2p2 doublet terms have equivalent electrons and the ionisation pathways are distributed between the 2 parents. Code : ADAS807 Producer : Martin O'Mullane Date : 19/12/00 ------------------------------------------------------------------------------- Add the orbital energies. Martin O'Mullane 12-12-2019 -------------------------------------------------------------------------------