CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Ti XI - 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]=6.00, 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)

543.5020 4.57e-01 2.06e+09 2.69e-04 4.91e-04 1.79e-03 3.64e-03 3s 3d 3D1 3p 3d 3F2 11 15 499858 683850
544.3980 1.07e-01 4.80e+08 6.26e-05 1.14e-04 4.17e-04 8.48e-04 3s 3d 3D2 3p 3d 3F2 12 15 500161 683850
551.3560 2.33e-10 1.02e+00 1.15e-02 4.07e-04 1.05e-08 3.81e-12 3s2 1S0 3s 3p 3P2 1 4 0 181371
569.0000 1.22e-03 8.32e+06 5.10e-02 5.52e-02 3.76e-02 1.82e-05 3s2 1S0 3s 3p 3P1 1 3 0 175747
618.4480 4.28e-02 1.50e+08 3.65e-05 4.08e-04 1.23e-03 3.49e-04 3s 3p 1P1 3p2 3P2 5 9 258972 420667
667.0760 3.30e-01 9.91e+08 8.93e-03 1.04e-02 1.46e-02 2.17e-03 3s 3p 1P1 3p2 1D2 5 6 258972 408880
768.4680 1.82e-01 4.08e+08 1.47e-05 2.01e-05 3.93e-05 4.99e-04 3s 3d 1D2 3p 3d 1D2 14 18 564613 694742
* 886.1760 3.98e+00 3.75e+09 2.32e-06 9.74e-06 2.34e-05 1.58e-03 3p 4p 3D3 3p 4d 3F4 57 70 1352524.8 1465369.2
* 943.7600 2.13e+00 2.27e+09 4.35e-06 7.87e-06 1.49e-05 9.82e-04 3s 4p 3P2 3s 4d 3D3 40 44 1136855.1 1242814.2

Created by Giulio Del Zanna on Wed Apr 16 17:44:33 2025