CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


O IV - VERSION 6.0


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]=5.20, 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)

617.0050 6.69e-02 2.94e+08 6.24e-04 6.42e-04 8.61e-04 7.49e-03 2s.2p2 2D3/2 2p3 2P3/2 6 15 126950.2 289023.5
617.0360 3.27e-01 2.88e+09 3.00e-03 3.10e-03 4.16e-03 3.66e-02 2s.2p2 2D3/2 2p3 2P1/2 6 14 126950.2 289015.4
624.6190 2.43e-01 1.00e+09 2.47e-04 4.87e-03 5.47e-02 4.34e-02 2s.2p2 4P1/2 2p3 4S3/2 3 11 71439.8 231537.5
625.1270 4.85e-01 2.00e+09 4.92e-04 9.71e-03 1.09e-01 8.64e-02 2s.2p2 4P3/2 2p3 4S3/2 4 11 71570.1 231537.5
625.8530 7.27e-01 2.98e+09 7.34e-04 1.45e-02 1.63e-01 1.29e-01 2s.2p2 4P5/2 2p3 4S3/2 5 11 71755.5 231537.5
779.7360 5.53e-02 1.52e+08 9.85e-04 1.03e-03 1.55e-03 4.25e-03 2s.2p2 2D5/2 2p3 2D3/2 7 12 126936.3 255184.9
779.8200 4.71e-01 1.29e+09 8.38e-03 8.73e-03 1.32e-02 3.62e-02 2s.2p2 2D3/2 2p3 2D3/2 6 12 126950.2 255184.9
779.9120 7.39e-01 1.35e+09 1.19e-02 1.26e-02 2.01e-02 5.66e-02 2s.2p2 2D5/2 2p3 2D5/2 7 13 126936.3 255155.9
779.9970 5.40e-02 9.90e+07 8.72e-04 9.21e-04 1.47e-03 4.14e-03 2s.2p2 2D3/2 2p3 2D5/2 6 13 126950.2 255155.9
787.7100 2.21e-01 5.98e+08 5.18e-01 5.18e-01 5.66e-01 5.32e-02 2s2.2p 2P1/2 2s.2p2 2D3/2 1 6 0 126950.2
790.1120 4.27e-02 1.15e+08 9.91e-02 9.91e-02 1.08e-01 1.02e-02 2s2.2p 2P3/2 2s.2p2 2D3/2 2 6 385.9 126950.2
790.1990 3.94e-01 7.06e+08 9.21e-01 9.33e-01 1.00e+00 9.39e-02 2s2.2p 2P3/2 2s.2p2 2D5/2 2 7 385.9 126936.3
802.2010 1.60e-01 4.16e+08 6.79e-04 6.98e-04 9.37e-04 8.15e-03 2s.2p2 2S1/2 2p3 2P3/2 8 15 164366.4 289023.5
802.2530 7.43e-02 3.86e+08 3.09e-04 3.20e-04 4.30e-04 3.78e-03 2s.2p2 2S1/2 2p3 2P1/2 8 14 164366.4 289015.4
921.2960 1.05e-01 2.08e+08 2.96e-04 3.04e-04 4.08e-04 3.55e-03 2s.2p2 2P1/2 2p3 2P3/2 9 15 180480.8 289023.5
921.3650 2.27e-01 8.95e+08 6.25e-04 6.46e-04 8.67e-04 7.64e-03 2s.2p2 2P1/2 2p3 2P1/2 9 14 180480.8 289015.4
923.3670 5.61e-01 1.10e+09 1.57e-03 1.61e-03 2.16e-03 1.88e-02 2s.2p2 2P3/2 2p3 2P3/2 10 15 180724.2 289023.5
923.4360 1.10e-01 4.34e+08 3.02e-04 3.13e-04 4.20e-04 3.70e-03 2s.2p2 2P3/2 2p3 2P1/2 10 14 180724.2 289015.4
1338.6140 2.35e-01 2.19e+08 8.27e-04 8.62e-04 1.30e-03 3.57e-03 2s.2p2 2P1/2 2p3 2D3/2 9 12 180480.8 255184.9
1342.9900 4.49e-02 4.16e+07 1.57e-04 1.63e-04 2.47e-04 6.76e-04 2s.2p2 2P3/2 2p3 2D3/2 10 12 180724.2 255184.9
1343.5140 4.16e-01 2.57e+08 1.32e-03 1.39e-03 2.22e-03 6.25e-03 2s.2p2 2P3/2 2p3 2D5/2 10 13 180724.2 255155.9
1397.2310 4.44e-08 3.75e+01 1.20e-02 7.34e-03 5.34e-07 3.10e-09 2s2.2p 2P1/2 2s.2p2 4P3/2 1 4 0 71570.1
1399.7800 8.76e-07 1.47e+03 2.64e-02 3.20e-02 1.05e-05 6.10e-08 2s2.2p 2P1/2 2s.2p2 4P1/2 1 3 0 71439.8
1401.1570 2.08e-06 1.16e+03 1.57e-01 1.59e-01 2.47e-05 1.44e-07 2s2.2p 2P3/2 2s.2p2 4P5/2 2 5 385.9 71755.5
1404.8060 3.47e-07 2.90e+02 9.25e-02 5.64e-02 4.10e-06 2.38e-08 2s2.2p 2P3/2 2s.2p2 4P3/2 2 4 385.9 71570.1
1407.3820 8.70e-07 1.45e+03 2.58e-02 3.12e-02 1.03e-05 5.96e-08 2s2.2p 2P3/2 2s.2p2 4P1/2 2 3 385.9 71439.8
* 4047.7429 1.60e+00 2.50e+09 1.33e-06 3.65e-06 3.57e-05 1.17e-03 2p2(3P).3p 4D7/2 2p2(3P).3d 4F9/2 123 71 594125.5 618830.62

Created by Giulio Del Zanna on Fri Sep 4 09:46:14 2009