CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Na VI - 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]=5.60, where the ion fraction peaks in ionization equilibrium. Only lines brighter than 0.001 the strongest line (at all densities) are retained. Lines flagged with a "*" before their wavelengths only have theoretical energy levels. Please note that their wavelengths are not very accurate.


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)

988.7090 1.16e-05 1.65e+04 1.23e-01 7.52e-02 4.41e-04 1.31e-07 2s2 2p2 3P2 2s 2p3 5S2 3 6 1856 102998
1356.3290 3.68e-09 1.34e+01 4.27e-02 9.80e-03 1.10e-07 1.68e-11 2s2 2p2 3P1 2s2 2p2 1S0 2 5 694.6 74423
* 1583.5840 1.51e+00 4.46e+08 1.69e-03 2.19e-03 2.01e-03 1.42e-04 2s2 2p 3p 3D3 2s2 2p 3d 3F4 28 41 867708 930855.9
1671.9611 1.12e+00 8.20e+08 6.95e-04 1.79e-03 1.67e-03 1.66e-04 2s2 2p 3s 1P1 2s2 2p 3p 1D2 24 33 817740 877550
2569.5510 3.31e-09 3.32e+00 5.60e-03 1.29e-03 1.45e-08 2.20e-12 2s2 2p2 1D2 2s2 2p2 1S0 4 5 35505.7 74423
2872.6470 2.65e-09 4.31e-01 5.58e-02 1.16e-03 1.17e-08 1.47e-12 2s2 2p2 3P1 2s2 2p2 1D2 2 4 694.6 35505.7
2971.7949 7.69e-09 1.17e+00 1.46e-01 3.05e-03 3.06e-08 3.87e-12 2s2 2p2 3P2 2s2 2p2 1D2 3 4 1856 35505.7
86102.9766 1.17e-07 2.09e-02 2.12e-02 2.90e-06 2.73e-11 2.72e-15 2s2 2p2 3P1 2s2 2p2 3P2 2 3 694.6 1856
143967.7500 5.66e-08 6.15e-03 7.40e-03 3.08e-07 2.91e-12 2.88e-16 2s2 2p2 3P0 2s2 2p2 3P1 1 2 0 694.6

Created by Giulio Del Zanna on Wed Apr 16 17:43:42 2025