CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.


P XII - VERSION 4.2


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]=6.30, 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)

278.2860 2.55e-01 7.31e+09 1.00e+00 1.00e+00 1.00e+00 1.00e+00 2s2 1S0/2 2s.2p 1P2/2 1 5 0 359343
288.3070 3.86e-03 6.19e+07 2.78e-04 3.03e-04 1.23e-03 1.19e-02 2s.2p 3P4/2 2p2 1D4/2 4 9 194856 541709
327.2310 1.26e-01 1.57e+09 1.33e-04 6.99e-03 2.21e-01 2.77e-01 2s.2p 3P2/2 2p2 3P4/2 3 8 187690 493285
327.5020 1.91e-01 1.19e+10 1.99e-03 2.04e-03 4.10e-03 3.65e-01 2s.2p 1P2/2 2p2 1S0/2 5 10 359343 664685
330.3330 9.97e-02 2.03e+09 1.73e-03 6.21e-03 1.80e-01 2.14e-01 2s.2p 3P0/2 2p2 3P2/2 2 7 184478 487203
333.8760 7.38e-02 1.47e+09 1.24e-03 4.45e-03 1.29e-01 1.53e-01 2s.2p 3P2/2 2p2 3P2/2 3 7 187690 487203
335.0890 3.65e-01 4.33e+09 3.57e-04 1.88e-02 5.95e-01 7.45e-01 2s.2p 3P4/2 2p2 3P4/2 4 8 194856 493285
338.4040 9.70e-02 5.65e+09 1.20e-04 1.88e-04 1.75e-01 1.94e-01 2s.2p 3P2/2 2p2 3P0/2 3 6 187690 483195
342.0600 1.20e-01 2.27e+09 1.87e-03 6.71e-03 1.94e-01 2.31e-01 2s.2p 3P4/2 2p2 3P2/2 4 7 194856 487203
532.7940 7.41e-05 5.80e+05 2.14e-01 2.13e-01 7.29e-02 4.79e-05 2s2 1S0/2 2s.2p 3P2/2 1 3 0 187690
548.3490 2.91e-01 1.29e+09 3.05e-03 3.33e-03 1.35e-02 1.31e-01 2s.2p 1P2/2 2p2 1D4/2 5 9 359343 541709

Created by Giulio Del Zanna on Fri Aug 5 13:56:20 2005