CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


O I - VERSION 11.0.1


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]=4.00, where the ion fraction peaks in ionization equilibrium. Only lines brighter than 0.001 the strongest line (at all densities) are retained.


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)

1302.1680 2.40e-01 3.15e+08 1.06e-03 7.49e-01 1.00e+00 1.00e+00 2s2.2p4 3P2 2s2.2p3(4S).3s 3S1 1 7 0 76794.978
1304.8580 1.44e-01 1.87e+08 6.29e-04 4.45e-01 5.94e-01 5.94e-01 2s2.2p4 3P1 2s2.2p3(4S).3s 3S1 2 7 158.265 76794.978
1306.0291 4.78e-02 6.23e+07 2.09e-04 1.48e-01 1.97e-01 1.97e-01 2s2.2p4 3P0 2s2.2p3(4S).3s 3S1 3 7 226.977 76794.978
1355.5980 1.98e-06 1.44e+03 1.45e-03 1.00e+00 6.38e-04 1.13e-05 2s2.2p4 3P2 2s2.2p3(4S).3s 5S2 1 6 0 73768.2
1358.5120 5.66e-07 4.09e+02 4.11e-04 2.84e-01 1.81e-04 3.21e-06 2s2.2p4 3P1 2s2.2p3(4S).3s 5S2 2 6 158.265 73768.2
2973.1541 0.00e+00 7.84e-02 4.33e-03 7.25e-02 9.99e-07 1.77e-08 2s2.2p4 3P1 2s2.2p4 1S0 2 5 158.265 33792.583
5578.8872 0.00e+00 1.26e+00 3.71e-02 6.21e-01 8.55e-06 1.52e-07 2s2.2p4 1D2 2s2.2p4 1S0 4 5 15867.862 33792.583
6302.0459 0.00e+00 6.50e-03 1.00e+00 1.89e-01 2.58e-06 4.56e-08 2s2.2p4 3P2 2s2.2p4 1D2 1 4 0 15867.862
6365.5361 0.00e+00 2.10e-03 3.20e-01 6.06e-02 8.24e-07 1.46e-08 2s2.2p4 3P1 2s2.2p4 1D2 2 4 158.265 15867.862
631851.6250 0.00e+00 8.54e-05 1.71e-03 1.43e-04 1.94e-09 3.44e-11 2s2.2p4 3P2 2s2.2p4 3P1 1 2 0 158.265

Created by Giulio Del Zanna on Wed Apr 16 17:44:06 2025