CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Ca IX - 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]=5.80, 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)

959.0760 1.92e-01 2.76e+08 1.28e-05 1.62e-05 4.47e-05 6.53e-04 3s 3d 1D2 3p 3d 1D2 14 18 467633 571900
* 1052.7920 3.16e+00 2.12e+09 4.72e-09 1.50e-08 7.95e-08 1.25e-03 3d 4p 3D3 3d 4d 3F4 117 183 1249881 1344866.5
* 1062.9930 6.04e+00 3.96e+09 3.33e-08 5.45e-08 2.08e-07 2.24e-03 3d 4p 1F3 3d 4d 1G4 124 188 1265053 1359127
* 1069.9240 1.73e+00 2.02e+09 7.24e-07 1.50e-06 7.87e-06 1.16e-03 3p 4p 3D1 3p 4d 3F2 55 74 1002258.9 1095723.5
* 1078.6110 1.84e+00 1.51e+09 4.56e-07 9.26e-07 4.03e-06 1.21e-03 3p 4p 3D2 3p 4d 3F3 56 75 1003546.8 1096258.6
* 1087.0861 4.59e+00 2.87e+09 2.67e-06 8.28e-06 3.33e-05 2.91e-03 3p 4p 3D3 3p 4d 3F4 57 76 1006737.4 1098726.4
1116.0710 1.63e+00 1.64e+09 3.77e-05 3.95e-05 5.23e-05 1.36e-03 3s 4p 1P1 3s 4d 1D2 32 45 832314 921914
* 1143.6260 1.25e+00 1.28e+09 4.44e-06 5.78e-06 1.77e-05 1.04e-03 3s 4p 3P1 3s 4d 3D2 30 43 827836.1 915277.3
* 1156.9120 2.52e+00 1.79e+09 8.21e-06 1.28e-05 3.51e-05 2.02e-03 3s 4p 3P2 3s 4d 3D3 31 44 829066.9 915503.9

Created by Giulio Del Zanna on Wed Apr 16 17:42:35 2025