CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


K V - 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]=5.30, 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)

2494.9980 0.00e+00 5.19e+00 1.00e+00 1.00e+00 1.00e+00 1.00e+00 3s2.3p3 4S3/2 3s2.3p3 2P3/2 1 5 0 40080.199
2515.2109 0.00e+00 2.14e+00 4.50e-01 2.06e-01 2.05e-01 2.05e-01 3s2.3p3 4S3/2 3s2.3p3 2P1/2 1 4 0 39758.1
4123.7788 0.00e+00 4.59e-03 1.22e-01 9.12e-04 9.00e-04 9.00e-04 3s2.3p3 4S3/2 3s2.3p3 2D5/2 1 3 0 24249.6
4164.4980 0.00e+00 8.84e-02 9.05e-01 1.16e-02 1.15e-02 1.15e-02 3s2.3p3 4S3/2 3s2.3p3 2D3/2 1 2 0 24012.5
6223.6670 0.00e+00 1.86e+00 1.44e-01 1.44e-01 1.44e-01 1.44e-01 3s2.3p3 2D3/2 3s2.3p3 2P3/2 2 5 24012.5 40080.199
6316.8799 0.00e+00 1.21e+00 9.21e-02 9.21e-02 9.21e-02 9.21e-02 3s2.3p3 2D5/2 3s2.3p3 2P3/2 3 5 24249.6 40080.199
6350.9810 0.00e+00 1.25e+00 1.04e-01 4.77e-02 4.74e-02 4.74e-02 3s2.3p3 2D3/2 3s2.3p3 2P1/2 2 4 24012.5 39758.1
6448.0771 0.00e+00 1.41e-01 1.16e-02 5.30e-03 5.27e-03 5.27e-03 3s2.3p3 2D5/2 3s2.3p3 2P1/2 3 4 24249.6 39758.1

Created by Giulio Del Zanna on Wed Apr 16 17:43:23 2025