CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Ne VI - VERSION 4.2


Here you find various information on the brightest lines, ordered in wavelength:
Wavelengths (Angstroms); weighted oscillator strengths (gf); transition probabilities (A); intensities (normalised) at 106 , 1010, 1015, 1020 cm-3; together with:
Configuration; Term; Index of the level (1=ground); Energy (observed if available - otherwise theoretical); of the lower (l) and upper levels (u)
Note that intensities have been calculated at log T[K]=5.60, where the ion fraction peaks in ionization equilibrium. Only lines brighter than 0.001 the strongest line (at all densities) are retained. Lines flagged with a "*" before their wavelengths only have theoretical energy levels. Please note that their wavelengths are not very accurate.


Wavelength

gf

Aul

R

R

R

R

Cl

Tl

Cu

Tu

Il

Iu

El

Eu

(A)

(s-1)

(106)

(1010)

(1015)

(1020)

(cm-1)

(cm-1)

440.4110 4.38e-01 3.76e+09 8.61e-03 6.99e-03 1.03e-02 2.79e-02 2s.2p2 2D5/2 2p3 2P3/2 7 15 178992 406053
440.4690 5.28e-02 4.53e+08 1.04e-03 8.42e-04 1.24e-03 3.36e-03 2s.2p2 2D3/2 2p3 2P3/2 6 15 179022 406053
440.5570 2.49e-01 4.28e+09 5.70e-03 3.96e-03 5.88e-03 1.59e-02 2s.2p2 2D3/2 2p3 2P1/2 6 14 179022 406008
451.8370 1.94e-01 1.57e+09 4.99e-04 6.66e-04 5.85e-02 1.64e-02 2s.2p2 4P1/2 2p3 4S3/2 3 11 100298 321617
452.7460 3.88e-01 3.15e+09 9.99e-04 1.33e-03 1.17e-01 3.29e-02 2s.2p2 4P3/2 2p3 4S3/2 4 11 100742 321617
454.0780 5.82e-01 4.72e+09 1.49e-03 1.99e-03 1.75e-01 4.91e-02 2s.2p2 4P5/2 2p3 4S3/2 5 11 101390 321617
553.6500 4.93e-02 2.71e+08 1.37e-03 8.82e-04 1.55e-03 1.98e-03 2s.2p2 2D5/2 2p3 2D3/2 7 12 178992 359612
553.7420 3.95e-01 2.17e+09 1.09e-02 7.06e-03 1.24e-02 1.59e-02 2s.2p2 2D3/2 2p3 2D3/2 6 12 179022 359612
553.8610 6.25e-01 2.29e+09 1.28e-02 1.15e-02 1.95e-02 2.51e-02 2s.2p2 2D5/2 2p3 2D5/2 7 13 178992 359543
553.9530 4.73e-02 1.73e+08 9.66e-04 8.69e-04 1.47e-03 1.90e-03 2s.2p2 2D3/2 2p3 2D5/2 6 13 179022 359543
558.5920 1.81e-01 9.58e+08 7.86e-01 3.81e-01 4.26e-01 1.38e-02 2s2.2p 2P1/2 2s.2p2 2D3/2 1 6 0 179022
562.7030 3.36e-02 1.78e+08 1.45e-01 7.03e-02 7.85e-02 2.55e-03 2s2.2p 2P3/2 2s.2p2 2D3/2 2 6 1308 179022
562.7980 3.21e-01 1.13e+09 5.42e-01 6.67e-01 7.24e-01 2.43e-02 2s2.2p 2P3/2 2s.2p2 2D5/2 2 7 1308 178992
570.7840 1.51e-01 7.74e+08 1.37e-03 1.11e-03 1.64e-03 4.43e-03 2s.2p2 2S1/2 2p3 2P3/2 8 15 230855 406053
570.9300 6.31e-02 6.46e+08 6.64e-04 4.61e-04 6.84e-04 1.86e-03 2s.2p2 2S1/2 2p3 2P1/2 8 14 230855 406008
637.8700 7.82e-02 3.18e+08 5.03e-04 4.08e-04 6.03e-04 1.63e-03 2s.2p2 2P1/2 2p3 2P3/2 9 15 249281 406053
638.0530 2.01e-01 1.64e+09 1.51e-03 1.05e-03 1.55e-03 4.21e-03 2s.2p2 2P1/2 2p3 2P1/2 9 14 249281 406008
641.2570 4.85e-01 1.97e+09 3.10e-03 2.51e-03 3.72e-03 1.00e-02 2s.2p2 2P3/2 2p3 2P3/2 10 15 250109 406053
641.4420 9.33e-02 7.58e+08 6.94e-04 4.81e-04 7.15e-04 1.94e-03 2s.2p2 2P3/2 2p3 2P1/2 10 14 250109 406008
906.3650 2.17e-01 4.44e+08 1.37e-03 8.82e-04 1.55e-03 1.98e-03 2s.2p2 2P1/2 2p3 2D3/2 9 12 249281 359612
913.2190 3.98e-02 8.14e+07 2.49e-04 1.61e-04 2.82e-04 3.61e-04 2s.2p2 2P3/2 2p3 2D3/2 10 12 250109 359612
913.7940 3.82e-01 5.21e+08 1.76e-03 1.59e-03 2.69e-03 3.46e-03 2s.2p2 2P3/2 2p3 2D5/2 10 13 250109 359543
992.6360 1.78e-07 3.01e+02 7.14e-03 4.80e-03 5.12e-06 3.19e-09 2s2.2p 2P1/2 2s.2p2 4P3/2 1 4 0 100742
997.0310 7.57e-06 1.27e+04 2.22e-02 1.36e-02 1.08e-04 6.71e-08 2s2.2p 2P1/2 2s.2p2 4P1/2 1 3 0 100298
999.1820 8.87e-06 9.87e+03 8.35e-02 7.67e-02 2.48e-04 1.56e-07 2s2.2p 2P3/2 2s.2p2 4P5/2 2 5 1308 101390
1005.6940 1.70e-06 2.80e+03 6.56e-02 4.41e-02 4.70e-05 2.93e-08 2s2.2p 2P3/2 2s.2p2 4P3/2 2 4 1308 100742
1010.2050 3.40e-06 1.11e+04 1.91e-02 1.17e-02 9.30e-05 5.79e-08 2s2.2p 2P3/2 2s.2p2 4P1/2 2 3 1308 100298
* 2751.8320 1.60e+00 4.71e+09 2.58e-06 2.69e-06 9.06e-05 1.03e-03 2p2(3P).3p 4D7/2 2p2(3P).3d 4F9/2 123 71 1053564.9 1089904.4
76452.7422 0.00e+00 2.09e-02 1.65e-02 2.40e-06 2.32e-11 4.16e-15 2s2.2p 2P1/2 2s2.2p 2P3/2 1 2 0 1308

Created by Giulio Del Zanna on Fri Aug 5 13:56:00 2005