CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Ca V - VERSION 6.0


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]=5.30, 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)

2281.2041 0.00e+00 1.22e-01 1.81e-03 5.52e-03 5.52e-03 5.52e-03 3s2.3p4 3P4/2 3s2.3p4 1S0/2 1 5 0 43836.5
2413.6050 0.00e+00 2.35e+01 3.28e-01 1.00e+00 1.00e+00 1.00e+00 3s2.3p4 3P2/2 3s2.3p4 1S0/2 2 5 2404.7 43836.5
3999.0081 0.00e+00 3.70e+00 3.12e-02 9.52e-02 9.52e-02 9.52e-02 3s2.3p4 1D4/2 3s2.3p4 1S0/2 4 5 18830.3 43836.5
5310.5898 0.00e+00 1.96e+00 1.00e+00 2.43e-01 2.27e-01 2.27e-01 3s2.3p4 3P4/2 3s2.3p4 1D4/2 1 4 0 18830.3
6088.0571 0.00e+00 4.36e-01 1.94e-01 4.73e-02 4.41e-02 4.41e-02 3s2.3p4 3P2/2 3s2.3p4 1D4/2 2 4 2404.7 18830.3
41585.2305 0.00e+00 3.08e-01 3.49e-01 3.43e-03 3.08e-03 3.08e-03 3s2.3p4 3P4/2 3s2.3p4 3P2/2 1 2 0 2404.7
114823.7266 0.00e+00 3.68e-02 1.44e-02 4.87e-05 4.42e-05 4.42e-05 3s2.3p4 3P2/2 3s2.3p4 3P0/2 2 3 2404.7 3275.6

Created by Giulio Del Zanna on Fri Sep 4 09:44:45 2009