CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


Mn VIII - 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]=5.80, 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)

185.4550 4.31e+00 3.01e+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 539214
235.4930 0.00e+00 2.29e+01 2.26e-03 4.11e-03 2.44e-07 1.39e-10 3s2.3p6 1S0/2 3s2.3p5.3d 3D4/2 1 9 0 424641
236.2190 4.69e-03 1.85e+08 3.91e-03 1.57e-02 3.36e-02 6.75e-04 3s2.3p6 1S0/2 3s2.3p5.3d 3D2/2 1 10 0 423337
238.1990 0.00e+00 8.28e+00 7.82e-04 1.41e-03 8.33e-08 5.04e-11 3s2.3p6 1S0/2 3s2.3p5.3d 1D4/2 1 11 0 419817
250.9010 0.00e+00 7.32e-01 3.95e-03 3.94e-04 6.47e-09 4.44e-12 3s2.3p6 1S0/2 3s2.3p5.3d 3F4/2 1 7 0 398564
263.1630 0.00e+00 6.02e+01 4.59e-02 2.53e-02 8.01e-07 3.64e-10 3s2.3p6 1S0/2 3s2.3p5.3d 3P4/2 1 4 0 379993
266.1630 3.92e-04 1.20e+07 1.21e-02 1.88e-02 2.21e-02 4.34e-05 3s2.3p6 1S0/2 3s2.3p5.3d 3P2/2 1 3 0 375710
2539.3000 0.00e+00 1.09e+01 1.11e-03 5.39e-04 1.68e-08 8.71e-12 3s2.3p5.3d 3P4/2 3s2.3p5.3d 3D6/2 4 8 379993 419374
2801.5181 0.00e+00 5.60e+01 1.02e-03 1.14e-03 7.71e-08 3.98e-11 3s2.3p5.3d 3F8/2 3s2.3p5.3d 1F6/2 5 12 391836 427531

Created by Giulio Del Zanna on Fri Sep 4 09:45:58 2009