chv6_ic#ca6.dat
Resolved Specific Ion Data Collections
- Ion
- Ca6+
- Temperature Range
- 2.111 eV → 2111 eV
ADF04
- Filename
- chv6_ic#ca6.dat
- Full Path
- adf04/copch#20/chv6_ic#ca6.dat
Download data
- Spontaneous Emission: Ca+6(i) → Ca+6(j) + hv
- Electron Impact Excitation: Ca+6(i) + e → Ca+6(j) + e
| 3s2.3p2 3p0 3P0.0 | 0.0 cm-1 |
| 3s2.3p2 3p1 3P1.0 | 1700.4 cm-1 |
| 3s2.3p2 3p2 3P2.0 | 4265.0 cm-1 |
| 3s2.3p2 1d2 1D2.0 | 24388.6 cm-1 |
| 3s2.3p2 1s0 1S0.0 | 50810.8 cm-1 |
| 3s.3p3 5s2 5S2.0 | 109858.0 cm-1 |
| 3s.3p3 3d1 3D1.0 | 159075.0 cm-1 |
| 3s.3p3 3d2 3D2.0 | 159141.0 cm-1 |
| 3s.3p3 3d3 3D3.0 | 159467.0 cm-1 |
| 3s.3p3 3p0 3P0.0 | 185508.0 cm-1 |
| 3s.3p3 3p2 3P2.0 | 185524.0 cm-1 |
| 3s.3p3 3p1 3P1.0 | 185534.0 cm-1 |
| 3s.3p3 1d2 1D2.0 | 204917.0 cm-1 |
| 3s.3p3 3s1 3S1.0 | 250706.0 cm-1 |
| 3s2.3p3d 3f2 3F2.0 | 251294.0 cm-1 |
| 3s2.3p3d 3f3 3F3.0 | 252821.0 cm-1 |
| 3s2.3p3d 3f4 3F4.0 | 254954.0 cm-1 |
| 3s.3p3 1p1 1P1.0 | 259581.0 cm-1 |
| 3s2.3p3d 3p2 3P2.0 | 292080.0 cm-1 |
| 3s2.3p3d 3p1 3P1.0 | 293671.0 cm-1 |
| 3s2.3p3d 3p0 3P0.0 | 294409.0 cm-1 |
| 3s2.3p3d 1d2 1D2.0 | 296811.0 cm-1 |
| 3s2.3p3d 3d1 3D1.0 | 301840.0 cm-1 |
| 3s2.3p3d 3d2 3D2.0 | 302536.0 cm-1 |
| 3s2.3p3d 3d3 3D3.0 | 302999.0 cm-1 |
| 3s2.3p3d 1f3 1F3.0 | 334258.0 cm-1 |
| 3s2.3p3d 1p1 1P1.0 | 341654.0 cm-1 |
A+ 6 20 7 1088910.0 ---------------------------------------------------------------------------- Data generated from CHIANTI version 6.0 http://www.chianti.rl.ac.uk/ CHIANTI references ------------------ Energy levels : %observed energy levels: Fuhr, J.R., Kelleher, D.E., Martin, W.C., Musgrove, A., Sugar, J., Wiese, W.L., Dalton, G.R., Dragoset, R.A., Mohr, P.J., Olsen, K., Reader, J., Saloman, E.B., Sansonetti, C.J., Wiersma, G., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data %observed energy level 18: Kelly, R.L., 1987, J.Phys.Chem.Ref.Data, 16, Suppl.1 %Theoretical energy levels: Landi & Bhatia, 2003, ApJ, 589, 1075 %Comment: Theoretical energies are taken from the 25-configuration model of Landi & Bhatia 2003. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data collaboration % % E. Landi - Dec 2002 A-values levels : %filename: ca_7.wgfa %observed energy levels: Fuhr, J.R., Kelleher, D.E., Martin, W.C., Musgrove, A., Sugar, J., Wiese, W.L., Dalton, G.R., Dragoset, R.A., Mohr, P.J., Olsen, K., Reader, J., Saloman, E.B., Sansonetti, C.J., Wiersma, G., "NIST Atomic Spectra Database" Ver. 2.0, March 1999, NIST Physical Reference Data %observed energy level 18: Kelly, R.L., 1987, J.Phys.Chem.Ref.Data, 16, Suppl.1 %Theoretical energy levels: Landi & Bhatia, 2003, ApJ, 589, 1075 % Oscillator strengths and A values: Landi & Bhatia, 2003, ApJ, 589, 1075 %Comment: theoretical energies, osc. strengths and A values are taken from the 25-configuration model of Landi & Bhatia 2003. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data collaboration % % E. Landi - Dec 2002 Collision strengths : %filename: ca_7.splups %oscillator strengths: Landi & Bhatia 2003, ApJ, 589, 1075 %collision strengths: Landi & Bhatia 2003, ApJ, 589, 1075 %comment: oscillator strengths are from the 5-configuration models in Landi & Bhatia 2003, for consistency with the atomic model in the collision problem % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Enrico Landi - Dec 2002 Added to ADAS by ---------------- Author : Martin O'Mullane Date : 28/10/10 ---------------------------------------------------------------------------- Unphysical A values. Set A=1.0E-30 for following transitions : 15 18 A = 4.16E-06 16 18 A = 5.72E-09 ------------------------------------------------------------------------------- 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 Original level order : 1 2 3 4 5 6 7 8 9 10 12 11 13 18 14 15 16 17 21 20 19 22 23 24 25 26 27 ------------------------------------------------------------------------------- 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 : ADAS utility program, filter04 Date : 28-10-2010 Producer : Martin O'Mullane ------------------------------------------------------------------------------- Regenerated to use the standard ADAS temperature set. Add the transitions in the CHIANTI source which have a transition probability but no accompanying effective collision strength and set these upsilons to zero. Update : Martin O'Mullane Date : 28-10-2010 -------------------------------------------------------------------------------