CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Fe XXII d - VERSION 5.1


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]=7.10, 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)

1.8752 3.45e-03 3.27e+12 3.49e-03 3.49e-03 3.49e-03 3.49e-03 2s2.2p 2P1/2 1s.2s2.2p2 2S1/2 1 24 0 53328966
1.8782 4.81e-03 2.27e+12 1.60e-03 1.60e-03 1.60e-03 1.60e-03 2s2.2p 2P1/2 1s.2s2.2p2 2P3/2 1 23 0 53244274
1.8794 2.80e-01 2.64e+14 2.81e-01 2.81e-01 2.81e-01 2.81e-01 2s2.2p 2P3/2 1s.2s2.2p2 2S1/2 2 24 118245.33 53328966
1.8812 2.63e-01 2.48e+14 3.25e-03 3.25e-03 3.25e-03 3.25e-03 2s.2p2 2P1/2 1s.2s.2p3(1P) 2P1/2 8 40 853689.33 54013756
1.8817 6.18e-01 5.82e+14 2.65e-03 2.65e-03 2.65e-03 2.65e-03 2s.2p2 2P3/2 1s.2s.2p3(3S) 2S1/2 10 42 992341.25 54138777
1.8824 6.34e-01 2.98e+14 6.80e-01 6.80e-01 6.80e-01 6.80e-01 2s2.2p 2P1/2 1s.2s2.2p2 2D3/2 1 21 0 53125706
1.8824 1.14e+00 5.35e+14 3.76e-01 3.76e-01 3.76e-01 3.76e-01 2s2.2p 2P3/2 1s.2s2.2p2 2P3/2 2 23 118245.33 53244274
1.8825 5.32e-01 5.00e+14 3.35e-02 3.35e-02 3.35e-02 3.35e-02 2s2.2p 2P1/2 1s.2s2.2p2 2P1/2 1 20 0 53124093
1.8832 4.28e-01 2.01e+14 7.99e-03 7.99e-03 7.99e-03 7.99e-03 2s.2p2 2P3/2 1s.2s.2p3(1P) 2P3/2 10 41 992341.25 54096834
1.8851 6.30e-01 1.97e+14 1.00e+00 1.00e+00 1.00e+00 1.00e+00 2s2.2p 2P3/2 1s.2s2.2p2 2D5/2 2 22 118245.33 53167649
1.8856 1.74e-01 1.63e+14 2.13e-03 2.13e-03 2.13e-03 2.13e-03 2s.2p2 2S1/2 1s.2s.2p3(1P) 2P1/2 9 40 978387.33 54013756
1.8858 7.32e-01 3.43e+14 2.06e-03 2.06e-03 2.06e-03 2.06e-03 2s.2p2 2D3/2 1s.2s.2p3(3D) 2D3/2 6 33 736331.24 53766941
1.8866 1.30e-01 6.07e+13 1.38e-01 1.38e-01 1.38e-01 1.38e-01 2s2.2p 2P3/2 1s.2s2.2p2 2D3/2 2 21 118245.33 53125706
1.8867 1.27e-01 1.19e+14 7.97e-03 7.97e-03 7.97e-03 7.97e-03 2s2.2p 2P3/2 1s.2s2.2p2 2P1/2 2 20 118245.33 53124093
1.8918 3.19e-02 2.97e+13 6.52e-03 6.52e-03 6.52e-03 6.52e-03 2s2.2p 2P1/2 1s.2s2.2p2 4P1/2 1 16 0 52863566
1.8919 8.34e-02 2.59e+13 3.20e-02 3.20e-02 3.20e-02 3.20e-02 2s2.2p 2P3/2 1s.2s2.2p2 4P5/2 2 18 118245.33 52978101
1.9288 3.93e-03 1.76e+12 1.21e-03 1.21e-03 1.21e-03 1.21e-03 2p3 2D3/2 1s.2s2.2p2 2P3/2 12 23 1396198.2 53244274
1.9299 1.10e-02 4.91e+12 3.37e-03 3.37e-03 3.37e-03 3.37e-03 2p3 2D5/2 1s.2s2.2p2 2P3/2 13 23 1426606.5 53244274
1.9316 4.63e-03 1.38e+12 6.84e-03 6.84e-03 6.84e-03 6.84e-03 2p3 2D3/2 1s.2s2.2p2 2D5/2 12 22 1396198.2 53167649
1.9321 5.05e-03 4.51e+12 4.67e-03 4.67e-03 4.67e-03 4.67e-03 2p3 2P1/2 1s.2s2.2p2 2S1/2 14 24 1569694.6 53328966
1.9328 1.63e-02 4.84e+12 2.40e-02 2.40e-02 2.40e-02 2.40e-02 2p3 2D5/2 1s.2s2.2p2 2D5/2 13 22 1426606.5 53167649
1.9332 4.60e-03 2.05e+12 4.55e-03 4.55e-03 4.55e-03 4.55e-03 2p3 2D3/2 1s.2s2.2p2 2D3/2 12 21 1396198.2 53125706
1.9335 1.29e-02 3.84e+12 4.64e-03 4.64e-03 4.64e-03 4.64e-03 2p3 4S3/2 1s.2s2.2p2 4P5/2 11 18 1255771.8 52978101
1.9343 9.23e-03 4.11e+12 9.12e-03 9.12e-03 9.12e-03 9.12e-03 2p3 2D5/2 1s.2s2.2p2 2D3/2 13 21 1426606.5 53125706
1.9343 4.17e-03 3.72e+12 3.85e-03 3.85e-03 3.85e-03 3.85e-03 2p3 2P3/2 1s.2s2.2p2 2S1/2 15 24 1627768.7 53328966
1.9374 9.32e-03 4.14e+12 2.83e-03 2.83e-03 2.83e-03 2.83e-03 2p3 2P3/2 1s.2s2.2p2 2P3/2 15 23 1627768.7 53244274
1.9397 2.51e-03 1.11e+12 2.46e-03 2.46e-03 2.46e-03 2.46e-03 2p3 2P1/2 1s.2s2.2p2 2D3/2 14 21 1569694.6 53125706
1.9403 1.55e-03 4.58e+11 2.26e-03 2.26e-03 2.26e-03 2.26e-03 2p3 2P3/2 1s.2s2.2p2 2D5/2 15 22 1627768.7 53167649

Created by Giulio Del Zanna on Wed Sep 14 15:43:37 2005