CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Cr VII - 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]=5.70, 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)

202.8260 4.69e+00 2.75e+11 1.00e+00 1.00e+00 1.00e+00 1.00e+00 3s2.3p6 1S0/2 3s2.3p5.3d 1P2/2 1 13 0 493035.4
258.6550 0.00e+00 1.71e+01 3.36e-03 4.87e-03 1.69e-07 1.17e-10 3s2.3p6 1S0/2 3s2.3p5.3d 3D4/2 1 9 0 386616.6
259.1830 3.74e-03 1.23e+08 4.04e-03 2.17e-02 4.11e-02 5.01e-04 3s2.3p6 1S0/2 3s2.3p5.3d 3D2/2 1 10 0 385828.3
261.3140 0.00e+00 7.03e+00 1.36e-03 1.96e-03 6.57e-08 4.80e-11 3s2.3p6 1S0/2 3s2.3p5.3d 1D4/2 1 11 0 382682.3
275.4360 0.00e+00 3.79e-01 4.77e-03 2.02e-04 3.23e-09 2.59e-12 3s2.3p6 1S0/2 3s2.3p5.3d 3F4/2 1 7 0 363060.9
288.9030 0.00e+00 4.46e+01 5.35e-02 2.30e-02 5.57e-07 3.06e-10 3s2.3p6 1S0/2 3s2.3p5.3d 3P4/2 1 4 0 346137.1
291.7380 3.51e-04 8.92e+06 1.47e-02 2.44e-02 2.38e-02 3.68e-05 3s2.3p6 1S0/2 3s2.3p5.3d 3P2/2 1 3 0 342773.5
2732.2229 0.00e+00 6.75e+00 1.35e-03 4.20e-04 9.74e-09 6.16e-12 3s2.3p5.3d 3P4/2 3s2.3p5.3d 3D6/2 4 8 346137.1 382737.4
3156.3220 0.00e+00 2.97e+01 1.15e-03 1.04e-03 3.65e-08 2.30e-11 3s2.3p5.3d 3F8/2 3s2.3p5.3d 1F6/2 5 12 357543.7 389226.2

Created by Giulio Del Zanna on Fri Sep 4 09:44:52 2009