helike_mom97#c4.dat
Resolved Specific Ion Data Collections
- Ion
- C4+
- Temperature Range
- 2.154 eV → 1.077 x 104 eV
ADF04
- Filename
- helike_mom97#c4.dat
- Full Path
- adf04/helike/helike_mom97#c4.dat
Download data
- Spontaneous Emission: C+4(i) → C+4(j) + hv
- Electron Impact Excitation: C+4(i) + e → C+4(j) + e
- Free Electron Recombination: C+5(i) + e → C+4(j)
| 1s2 1S0.0 | 0.0 cm-1 |
| 1s1 2s1 3S1.0 | 2411260.0 cm-1 |
| 1s1 2s1 1S0.0 | 2455020.0 cm-1 |
| 1s1 2p1 3P4.0 | 2455220.0 cm-1 |
| 1s1 2p1 1P1.0 | 2483370.0 cm-1 |
| 1s1 3s1 3S1.0 | 2839560.0 cm-1 |
| 1s1 3s1 1S0.0 | 2851180.0 cm-1 |
| 1s1 3p1 3P4.0 | 2851420.0 cm-1 |
| 1s1 3d1 3D7.0 | 2857310.0 cm-1 |
| 1s1 3d1 1D2.0 | 2857530.0 cm-1 |
| 1s1 3p1 1P1.0 | 2859380.0 cm-1 |
| 1s1 4s1 3S1.0 | 2983540.0 cm-1 |
| 1s1 4s1 1S0.0 | 2988460.0 cm-1 |
| 1s1 4p1 3P4.0 | 2988360.0 cm-1 |
| 1s1 4d1 3D7.0 | 2990780.0 cm-1 |
| 1s1 4d1 1D2.0 | 2990920.0 cm-1 |
| 1s1 4f1 1F3.0 | 2990920.0 cm-1 |
| 1s1 4f1 3F10.0 | 2990920.0 cm-1 |
| 1s1 4p1 1P1.0 | 2991710.0 cm-1 |
| 1s1 5s1 3S1.0 | 3048930.0 cm-1 |
| 1s1 5p1 3P4.0 | 3051330.0 cm-1 |
| 1s1 5s1 1S0.0 | 3051440.0 cm-1 |
| 1s1 5d1 3D7.0 | 3052590.0 cm-1 |
| 1s1 5d1 1D2.0 | 3052660.0 cm-1 |
| 1s1 5g1 1G4.0 | 3052660.0 cm-1 |
| 1s1 5f1 3F10.0 | 3052650.0 cm-1 |
| 1s1 5f1 1F3.0 | 3052650.0 cm-1 |
| 1s1 5g1 3G13.0 | 3052660.0 cm-1 |
| 1s1 5p1 1P1.0 | 3053040.0 cm-1 |
Predecessors
Contributors
- Martin O'Mullane
- Douglas Sampson
- Keith Berrington
- Harvey Anderson
- Nigel Badnell
+ 4 6 5 3162395.0(2S) ------------------------------------------------------------------------------- Combined two specific ion files Target : JETXPQ.COPMM#HE.DATA(C4#LS#A) Supplementary : JETXPQ.COPMM#HE.DATA(HA#C4) 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 18 18 17 19 19 20 20 21 22 22 21 23 23 24 26 25 27 26 24 27 28 28 25 29 29 Code : JETXPQ.ATS.FORT(CADF04) 16:44 28/10/1997 ------------------------------------------------------------------------------- Update A values of following transitions from the supplementary file 7 1, 9 1, 10 1, 13 1, 15 1, 16 1, 22 1, 23 1 24 1, 6 2, 9 2, 10 2, 12 2, 15 2, 16 2, 20 2 23 2, 24 2, 28 2, 7 3, 9 3, 10 3, 13 3, 15 3 16 3, 22 3, 23 3, 24 3, 12 6, 15 6, 16 6, 20 6 23 6, 24 6, 28 6, 13 7, 15 7, 16 7, 22 7, 23 7 24 7, 12 9, 15 9, 16 9, 20 9, 23 9, 24 9, 28 9 13 9, 22 9, 25 9, 12 10, 13 10, 15 10, 16 10, 20 10 22 10, 23 10, 24 10, 28 10, 25 10, 20 12, 23 12, 24 12 28 12, 22 13, 23 13, 24 13, 20 15, 23 15, 24 15, 28 15 22 15, 25 15, 20 16, 22 16, 23 16, 24 16, 28 16, 25 16 8 4, 14 4, 18 4, 21 4, 26 4, 11 4, 17 4, 19 4 27 4, 29 4, 8 5, 11 5, 14 5, 18 5, 17 5, 19 5 21 5, 26 5, 27 5, 29 5, 14 8, 18 8, 21 8, 26 8 17 8, 19 8, 27 8, 29 8, 14 11, 18 11, 17 11, 19 11 21 11, 26 11, 27 11, 29 11, 21 14, 26 14, 27 14, 29 14 21 18, 29 18, 21 17, 26 17, 29 17, 21 19, 26 19, 27 19 29 19, 8 1, 14 1, 21 1, 11 2, 18 2, 19 2, 26 2 29 2, 8 3, 14 3, 21 3, 6 5, 14 6, 18 6, 19 6 21 6, 26 6, 29 6, 7 4, 7 5, 14 7, 21 7, 9 5 14 9, 18 9, 19 9, 21 9, 26 9, 29 9, 17 9, 27 9 10 4, 14 10, 18 10, 17 10, 21 10, 26 10, 27 10, 12 4 12 5, 12 8, 12 11, 21 12, 26 12, 29 12, 13 4, 13 5 13 8, 13 11, 21 13, 29 13, 15 4, 15 5, 15 8, 15 11 21 15, 26 15, 29 15, 27 15, 16 4, 16 5, 16 8, 16 11 21 16, 26 16, 27 16, 20 4, 20 5, 20 8, 20 11, 20 14 20 18, 20 19, 22 4, 22 5, 22 8, 22 11, 22 14, 22 19 23 4, 23 5, 23 8, 23 11, 23 14, 23 18, 23 19, 23 17 24 4, 24 5, 24 8, 24 11, 24 14, 24 18, 24 17, 24 19 28 4, 28 8, 28 14 Martin O'Mullane 28-10-97 --------------------------------------------------------------------------------- Comments from target file --------------------------------------------------------------------------------- Generated from Cowan Atomic Structure Program M O'Mullane 17:56 22/10/1997 SCF method used : HR Scale factors for Slater Parameters : 85 97 85 90 85 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 : 12,all Parity 1 Parity 2 Allowed 372 373 606 initially 186 130 290 reduced --------------------------------------------------------------------------------- Comments from supplementary file ------------------------------------------------------------------------------- Specific ion file based on effective collision strength data of Sampson and co-workers Energies : NIST Standard Reference Database 61 A-values : NIST Standard Reference Database 61 and Opacity Project (Berrington et al.) Upsilons : Fits of Golden et. al(1981)Ap.J.Suppl.45, 603 & (1978) Ap.J. Suppl.38,19; extended and revised by Clark (1982)Ap. J. Supple. 49,545. Generating code: jetand.copase.fort(samp#he) Producer: H. Anderson Date: 24/07/96 ------------------------------------------------------------------------------- SUPPLEMENTARY DATA , SEE REFERENCE (1), WAS USED TO ADJUST THE UPSILONS FOR 1-2,1-3,1-4 AND 1-5. IN THE LITERATURE, THIS DATA IS REPRESENTED AS ANALYTICAL FORMULAE AND IS REPORTED TO BE VALID OVER A FINITE TEMPERATURE RANGE. THEREFORE THE TREATMENT OUTLINED IN REFERENCE (2) WAS USED TO EXTEND THE TEMPERATURE RANGE OF THE DATA. REFERENCES (1) KATO.T AND NAKAZAKI.S ATOMIC DATA AND NUCLEAR DATA TABLES 42,313-338 ( 1989 ). (2) BURGESS.A AND TULLY.J.A ASTRON. ASTROPHYS. 254, 436-453 (1992) H ANDERSON 24/07/96 ------------------------------------------------------------------------------- RADIATIVE RECOMBINATION DATA ADDED PROCESSED BY ADAS211 ON : /home/mog/adas/adf08/rrc96#h/rrc96#h_c5ls.dat Martin O'Mullane 28-10-97 ------------------------------------------------------------------------------- Dielectronic data is post-processed from Badnell files as follows: /u/adas/adas/adf09/mom96#h/mom96#h_c5ls12.dat The cross-referencing file is as follows: /home/mog/adas/adf18/a09_a04/mom96#he/mom96#he_c4ls.dat The parent metastable indices are as follows: 1. 1S1 (2)0( 0.5) Dielectronic data added to 29 existing rad. recom. level sets Martin O'Mullane 28-10-97 ------------------------------------------------------------------------------- --------------------------------------------------------------------------------- ---------------------------------------------------------------------------------