CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Cl III - 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]=4.65, 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)

3343.7600 0.00e+00 7.54e-01 1.00e+00 1.00e+00 1.00e+00 1.00e+00 3s2.3p3 4S3/2 3s2.3p3 2P3/2 1 5 0 29906.45
3354.1379 0.00e+00 3.05e-01 3.69e-01 2.02e-01 2.02e-01 2.02e-01 3s2.3p3 4S3/2 3s2.3p3 2P1/2 1 4 0 29813.92
5519.2422 0.00e+00 7.05e-04 1.94e-02 1.24e-03 1.24e-03 1.24e-03 3s2.3p3 4S3/2 3s2.3p3 2D5/2 1 3 0 18118.43
5539.4111 0.00e+00 4.84e-03 9.57e-02 5.68e-03 5.67e-03 5.67e-03 3s2.3p3 4S3/2 3s2.3p3 2D3/2 1 2 0 18052.46
8435.9775 0.00e+00 3.23e-01 1.70e-01 1.70e-01 1.70e-01 1.70e-01 3s2.3p3 2D3/2 3s2.3p3 2P3/2 2 5 18052.46 29906.45
8483.1895 0.00e+00 3.16e-01 1.65e-01 1.65e-01 1.65e-01 1.65e-01 3s2.3p3 2D5/2 3s2.3p3 2P3/2 3 5 18118.43 29906.45
8502.3457 0.00e+00 3.03e-01 1.45e-01 7.93e-02 7.93e-02 7.93e-02 3s2.3p3 2D3/2 3s2.3p3 2P1/2 2 4 18052.46 29813.92
8550.3037 0.00e+00 1.00e-01 4.74e-02 2.60e-02 2.60e-02 2.60e-02 3s2.3p3 2D5/2 3s2.3p3 2P1/2 3 4 18118.43 29813.92

Created by Giulio Del Zanna on Wed Apr 16 17:42:36 2025