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]=6.40, 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)

1018.7240

0.00e+00

2.42e+00

2.12e-02

5.52e-03

4.00e-07

9.41e-12

2s2.2p3

4S3/2

2s2.2p3

2D5/2

1

3

0

98162

1054.6851

0.00e+00

1.01e+02

2.20e-02

2.64e-02

1.10e-05

2.53e-10

2s2.2p3

4S3/2

2s2.2p3

2D3/2

1

2

0

94815

1688.1910

0.00e+00

4.31e+02

1.37e-03

2.84e-03

2.18e-05

6.20e-10

2s2.2p3

2D3/2

2s2.2p3

2P3/2

2

5

94815

154050

1789.2930

0.00e+00

2.14e+02

6.42e-04

1.33e-03

1.02e-05

2.90e-10

2s2.2p3

2D5/2

2s2.2p3

2P3/2

3

5

98162

154050

1839.5880

0.00e+00

2.15e+02

7.52e-04

1.19e-03

5.19e-06

1.43e-10

2s2.2p3

2D3/2

2s2.2p3

2P1/2

2

4

94815

149175

Created by Giulio Del Zanna on Wed Jun 8 16:01:08 2022