CHIANTI

An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.

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Naval Research Laboratory (USA) - Rutherford Appleton Laboratory (UK)
University of Cambridge (UK) - George Mason University (USA) - Universita' degli Studi di Firenze (Italy)

VERSION 4.2

H I
He I II
C II III IV V VI
N I II III IV V VI VII
O II III IV V VI VII VIII
Ne II III IV V VI VII VIII IX X
Na III IV V VI VII VIII IX X XI
Mg II IV V VI VII VIII IX X XI XII
Al III V VI VII VIII IX X XI XII XIII
Si II III IV V VI VII VIII IX X XI XII XIII XIV
P V VII VIII IX X XI XII XIII
S II III IV V VI VII VIII IX X XI XII XIII XIV XV XVI
Cl XIV
Ar IV VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII
K IX XI XII XIII XIV XV XVI XVII
Ca IX X XI XII XIII XIV XV XVI XVII XVIII XIX XX
Ti XI XII XIV XV XVI XVII XVIII XIX XX
Cr XIII XIV XVI XVII XVIII XIX XX XXI XXII
Mn XV XVII XVIII XIX XX XXI XXII XXIII
Fe II VI VII VIII IX X XI XII XIII XIV XV XVI XVII XVIII XIX XX XXI XXII XXIII XXIV XXV XXVI
Co XVII XIX XXI XXII XXIII XXIV XXV
Ni XII XIII XV XVI XVII XVIII XIX XX XXI XXII XXIII XXIV XXV XXVI XXVII XXVIII
Zn XX XXIV XXV XXVII XXVIII

Ions that produce satellite lines

C IV V
N V VI
O VI VII
Ne VIII IX
Mg X XI
Al XI XII
Si XII XIII
S XIV XV
Ar XVI XVII
Ca XVIII XIX
Fe XXI XXII XXIII XXIV XXV
Ni XXVI XXVII

Page designed and last modified by Giulio Del Zanna on Fri Aug 5 13:53:45 2005
Last revised by G. Del Zanna on 4-Sep-2009