CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Ne X - 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]=6.65, 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)

9.3616 9.81e-03 1.87e+11 9.55e-03 9.55e-03 9.64e-03 1.07e-02 1s 2S1/2 6p 2P3/2 1 28 0 10681954
9.3617 4.84e-03 1.84e+11 4.76e-03 4.76e-03 4.81e-03 5.33e-03 1s 2S1/2 6p 2P1/2 1 27 0 10681818
9.4807 1.81e-02 3.36e+11 1.77e-02 1.77e-02 1.79e-02 2.03e-02 1s 2S1/2 5p 2P3/2 1 19 0 10547772
9.4809 8.96e-03 3.33e+11 8.84e-03 8.84e-03 8.94e-03 1.01e-02 1s 2S1/2 5p 2P1/2 1 18 0 10547537
9.7080 3.81e-02 6.74e+11 4.03e-02 4.03e-02 4.09e-02 4.82e-02 1s 2S1/2 4p 2P3/2 1 12 0 10300749
9.7085 1.89e-02 6.69e+11 2.01e-02 2.01e-02 2.04e-02 2.41e-02 1s 2S1/2 4p 2P1/2 1 11 0 10300290
10.2385 1.05e-01 1.67e+12 1.29e-01 1.29e-01 1.34e-01 1.84e-01 1s 2S1/2 3p 2P3/2 1 7 0 9767062.9
10.2396 5.21e-02 1.66e+12 6.46e-02 6.46e-02 6.69e-02 9.19e-02 1s 2S1/2 3p 2P1/2 1 6 0 9765974.6
12.1321 5.52e-01 6.26e+12 1.00e+00 1.00e+00 1.00e+00 1.00e+00 1s 2S1/2 2p 2P3/2 1 4 0 8242606
12.1375 2.76e-01 6.26e+12 5.00e-01 5.00e-01 5.00e-01 5.00e-01 1s 2S1/2 2p 2P1/2 1 3 0 8238933.4
43.3794 1.59e-01 9.41e+10 5.77e-04 5.77e-04 6.20e-04 1.08e-03 2p 2P3/2 5d 2D5/2 4 21 8242606 10547850
48.5010 2.43e-01 1.72e+11 6.91e-04 6.91e-04 7.69e-04 1.62e-03 2p 2P1/2 4d 2D3/2 3 13 8238933.4 10300748
48.5048 1.36e-01 9.62e+10 1.15e-03 1.15e-03 1.17e-03 1.38e-03 2s 2S1/2 4p 2P3/2 2 12 8239096.5 10300749
48.5839 4.38e-01 2.06e+11 1.23e-03 1.23e-03 1.37e-03 2.90e-03 2p 2P3/2 4d 2D5/2 4 14 8242606 10300901
48.5978 1.22e-02 1.72e+10 1.22e-03 1.22e-03 1.27e-03 1.67e-03 2p 2P3/2 4s 2S1/2 4 10 8242606 10300310
65.4400 1.39e+00 5.40e+11 1.84e-03 1.84e-03 2.45e-03 8.95e-03 2p 2P1/2 3d 2D3/2 3 8 8238933.4 9767061.1
65.4460 5.75e-01 2.24e+11 2.72e-03 2.72e-03 2.81e-03 3.87e-03 2s 2S1/2 3p 2P3/2 2 7 8239096.5 9767062.9
65.4840 2.69e-02 2.09e+10 2.46e-03 2.46e-03 2.67e-03 3.89e-03 2p 2P1/2 3s 2S1/2 3 5 8238933.4 9766023.4
65.4930 2.89e-01 2.25e+11 1.37e-03 1.37e-03 1.42e-03 1.95e-03 2s 2S1/2 3p 2P1/2 2 6 8239096.5 9765974.6
65.5820 2.50e+00 6.47e+11 3.29e-03 3.29e-03 4.38e-03 1.60e-02 2p 2P3/2 3d 2D5/2 4 9 8242606 9767422.9
65.5970 2.78e-01 1.08e+11 3.67e-04 3.67e-04 4.88e-04 1.78e-03 2p 2P3/2 3d 2D3/2 4 8 8242606 9767061.1
65.6420 5.50e-02 4.25e+10 4.99e-03 4.99e-03 5.42e-03 7.88e-03 2p 2P3/2 3s 2S1/2 4 5 8242606 9766023.4

Created by Giulio Del Zanna on Wed Apr 16 17:43:48 2025