CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Ca 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]=5.50, 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)

2215.1980 0.00e+00 1.13e+01 5.94e-01 1.00e+00 1.00e+00 1.00e+00 3s2.3p3 4S3/2 3s2.3p3 2P3/2 1 5 0 45142.7
2242.8210 0.00e+00 4.74e+00 2.69e-01 2.15e-01 2.08e-01 2.08e-01 3s2.3p3 4S3/2 3s2.3p3 2P1/2 1 4 0 44586.7
3670.1831 0.00e+00 1.16e-02 3.66e-01 1.09e-03 1.01e-03 1.01e-03 3s2.3p3 4S3/2 3s2.3p3 2D5/2 1 3 0 27246.6
3726.4629 0.00e+00 2.91e-01 1.00e+00 1.82e-02 1.66e-02 1.66e-02 3s2.3p3 4S3/2 3s2.3p3 2D3/2 1 2 0 26835.1
5462.2119 0.00e+00 4.06e+00 8.65e-02 1.46e-01 1.46e-01 1.46e-01 3s2.3p3 2D3/2 3s2.3p3 2P3/2 2 5 26835.1 45142.7
5587.8101 0.00e+00 2.39e+00 4.99e-02 8.40e-02 8.40e-02 8.40e-02 3s2.3p3 2D5/2 3s2.3p3 2P3/2 3 5 27246.6 45142.7
5633.2949 0.00e+00 2.51e+00 5.68e-02 4.53e-02 4.38e-02 4.38e-02 3s2.3p3 2D3/2 3s2.3p3 2P1/2 2 4 26835.1 44586.7
5766.9790 0.00e+00 1.64e-01 3.62e-03 2.89e-03 2.79e-03 2.79e-03 3s2.3p3 2D5/2 3s2.3p3 2P1/2 3 4 27246.6 44586.7

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