CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Mg II - 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]=4.15, 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)

1737.6281 1.39e-01 4.91e+07 5.79e-05 5.79e-05 5.47e-04 1.34e-03 3p 2P3/2 4d 2D5/2 3 11 35760.898 93310.602
2791.5959 1.93e+00 3.93e+08 2.42e-03 2.42e-03 1.85e-02 4.10e-02 3p 2P1/2 3d 2D3/2 2 5 35669.301 71491.102
2796.3501 1.27e+00 2.52e+08 1.00e+00 1.00e+00 1.00e+00 1.00e+00 3s 2S1/2 3p 2P3/2 1 3 0 35760.898
2798.7529 3.87e-01 7.82e+07 4.81e-04 4.81e-04 3.67e-03 8.14e-03 3p 2P3/2 3d 2D3/2 3 5 35760.898 71491.102
2798.8230 3.48e+00 4.69e+08 4.35e-03 4.35e-03 3.31e-02 7.33e-02 3p 2P3/2 3d 2D5/2 3 6 35760.898 71490.203
2803.5310 6.35e-01 2.51e+08 5.04e-01 5.04e-01 5.02e-01 5.01e-01 3s 2S1/2 3p 2P1/2 1 2 0 35669.301
2929.4929 2.96e-01 1.10e+08 1.18e-03 1.18e-03 3.18e-03 6.50e-03 3p 2P1/2 4s 2S1/2 2 4 35669.301 69804.898
2937.3750 5.94e-01 2.21e+08 2.36e-03 2.36e-03 6.37e-03 1.30e-02 3p 2P3/2 4s 2S1/2 3 4 35760.898 69804.898
4482.3950 5.64e+00 2.26e+08 4.60e-05 4.61e-05 1.23e-03 3.03e-03 3d 2D5/2 4f 2F7/2 6 13 71490.203 93799.703
4482.5962 3.95e+00 2.11e+08 3.21e-05 3.22e-05 8.61e-04 2.12e-03 3d 2D3/2 4f 2F5/2 5 12 71491.102 93799.602

Created by Giulio Del Zanna on Wed Apr 16 17:43:31 2025